Mathematical Elasticity Volume III: Theory of Shells [29, 1° ed.]
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MATHEMATICAL ELASTICITY VOLUME III: THEORY OF SHELLS

VOLUME

III: T H E O R Y

OF SHELLS

Part A. Linear shell theory Chapter

1. Three-dimensional linearized elasticity and Korn's inequalities in curvilinear coordinates

Chapter Chapter

2. Inequalities of Korn's type on surfaces 3. Asymptotic analysis of linearly elastic shells: Preliminaries and outline 4. Linearly elastic elliptic membrane shells 5. Linearly elastic generalized membrane shells 6. Linearly elastic flexural shells 7. Koiter's equations and other linear shell theories

Chapter Chapter Chapter Chapter

Part B. Nonlinear shell theory Chapter

8. Asymptotic analysis of nonlinearly elastic shells: Preliminaries Chapter 9. Nonlinearly elastic membrane shells Chapter 10. Nonlinearly elastic flexural shells Chapter 11. Koiter's equations and other nonlinear shell theories

MATHEMATICAL ELASTICITY V O L U M E III: T H E O R Y OF S H E L L S

PHILIPPE G. CIARLET Institut Universitaire de France Universitd Pierre et Marie Curie, Paris, France

With

31 f i g u r e s b y t h e a u t h o r

2000 ELSEVIER AMSTERDAM

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ELSEVIER SCIENCE B.V. Sara Burgerhartstraat 25 P.O. Box 211, 1000 AE Amsterdam, The Netherlands

9 2000 Elsevier Science B.V. All rights reserved. This w o r k is p r o t e c t e d u n d e r c o p y r i g h t by E l s e v i e r Science, and the f o l l o w i n g terms and c o n d i t i o n s a p p l y to its use: Photocopying Single photocopies of single chapters may be made for personal use as allowed by national copyright laws. Permission of the Publisher and payment of a fee is required for all other photocopying, including multiple or systematic copying, copying for advertising or promotional purposes, resale, and all forms of document delivery. Special rates are available for educational institutions that wish to make photocopies for non-profit educational classroom use. Permissions may be sought directly from Elsevier Science Rights & Permissions Department, PO Box 800, Oxford OX5 I DX, UK; phone: (+44) 1865 843830, fax: (+44) 1865 853333, e-mail: [email protected]. You may also contact Rights & Permissions directly through Elsevier's home page (http://www.elsevier.nl), selecting first 'Customer Support', then 'General Information', then 'Permissions Query Form'. In the USA, users may clear permissions and make payments through the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923, USA; phone: (978) 7508400, fax: (978) 7504744, and in the UK through the Copyright Licensing Agency Rapid Clearance Service (CLARCS), 90 Tottenham Court Road, London W I P 0LP, UK; phone: (+44) 171 631 5555; fax: (+44) 171 631 5500. Other countries may have a local reprographic rights agency for payments. Derivative Works Tables of contents may be reproduced for internal circulation, but permission of Elsevier Science is required for external resale or distribution of such material. Permission of the Publisher is required for all other derivative works, including compilations and translations. Electronic Storage or Usage Permission of the Publisher is required to store or use electronically any material contained in this work, including any chapter or part of a chapter. Except as outlined above, no part of this work may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without prior written permission of the Publisher. Address permissions requests to: Elsevier Science Rights & Permissions Department, at the mail, fax and e-mail addresses noted above. Notice No responsibility is assumed by the Publisher for any injury and/or damage to persons or property as a matter of products liability, negligence or otherwise, or from any use or operation of any methods, products, instructions or ideas contained in the material herein. Because of rapid advances in the medical sciences, in particular, independent verification of diagnoses and drug dosages should be made.

First edition 2000

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MATHEMATICAL PREFACE 1

ELASTICITY:

GENERAL

This treatise, which comprises three volumes, is intended to be b o t h a thorough introduction to contemporary research in elasticity and a working textbook at the graduate level for courses in pure or

applied mathematics or in continuum mechanics. During the past decades, elasticity has become the object of a considerable renewed interest, both in its physical foundations and in its m a t h e m a t i c a l theory. One reason behind this recent attention is that it has been increasingly acknowledged that the classical linear equations of elasticity, whose mathematical theory is now firmly established, have a limited range of applicability, outside of which they should be replaced by the genuine nonlinear equations that they in effect approximate. Another reason, similar in its principle, is that the validity of the classical lower-dimensional equations, such as the two-dimensional yon Ks equations for nonlinearly elastic plates or the twodimensional Koiter equations for linearly elastic shells, is no longer left unquestioned. A need has been felt for a better assessment of their relation to the corresponding three-dimensional equations that they are supposed to "replace". Thanks to the ever-increasing power of available computers, sophisticated mathematical models that were previously intractable by approximate methods are now amenable to numerical simulations. This is one more reason why these models should be established on firm grounds. This treatise illustrates at length these recent trends, as shown by the main topics covered: A thorough description, with a pervading emphasis on the nonlinear aspects, of the two existing mathematical models of threedimensional elasticity, either as a boundary value problem consisting of a system of three quasilinear partial differential equations of -

1This "General preface" is an updated excerpt from the "Preface" to the first edition (1988) of Volume I.

Mathematical Elasticity: Generalpreface

vi

the second order together with specific boundary conditions, or as a minimization problem for the associated energy over an ad hoc set of admissible deformations (Vol. I, Part A);

A mathematical analysis of these models, comprising in particular complete proofs of all the available existence results, relying either on the implicit function theorem, or on the direct methods of the calculus of variations (Vol. I, Part B); -

-

A mathematical justification of the well-known two-dimensional

linear Kirchhoff-Love theory of plates, by means of convergence theorems as the thickness of the plate approaches zero (Vol. II, Part A); Similar justifications of mathematical models of junctions in linearly elastic multi-structures and of linearly elastic shallow shells -

(Vol. II, Part A); - A systematic derivation of two-dimensional plate models from nonlinear three-dimensional elasticity by means of the method of formal asymptotic expansions, which includes a justification of wellknown plate models, such as the nonlinear Kirchhoff-Love theory and the yon Kdrmdn equations (Vol. II, Part B); - A derivation of the large de]ormation, frame-indifferent, nonlinear planar membrane and flexural theories by means of the method of formal asymptotic expansions and a justification of nonlinear planar membrane equations by means of a convergence theorem (Vol. II, Part B);

A mathematical analysis of the two-dimensional, linear and nonlinear, plate equations, which includes in particular a review of the existence and regularity theorems in the nonlinear case and an introduction to bifurcation theory (Vol. II, Parts A and B); -

- A mathematical justification by means of convergence theorems of the two-dimensional membrane, flexural, and Koiter equations of a linearly elastic shell (Vol. III, Part A); - A systematic derivation of the two-dimensional membrane and flexural equations o] a nonlinearly elastic shell by means of the method of formal asymptotic expansions and a justification of nonlinear membrane shell equations by means of a convergence theorem (Vol. III, Part B).

- A mathematical analysis of the two-dimensional, linear and nonlinear, shell equations, with a particular emphasis on the existence theory (Vol. III, Parts A and B).

Mathematical Elasticity: General preface

vii

Although the emphasis is definitely on the mathematical side, every effort has been made to keep the prerequisites, whether from mathematics or continuum mechanics, to a minimum, notably by making this treatise as largely self-contained as possible. Its reading only presupposes some familiarity with basic topics from analysis and functional analysis. Naturally, frequent references are made to Vol. I in Vol. II, and to Vols. I and II in Vol. III. However, I have also tried to render each volume as sel~-contained as possible. In particular, all relevant notions from three-dimensional elasticity are (at least briefly) recalled wherever they are needed in Vols. II and III. References are also made to Vol. I regarding various mathematical notions (properties of domains in ]Rn, differential calculus in normed vector spaces, Sobolev spaces, weak lower semi-continuity, etc.). This is a mere convenience, reflecting that I also regard the three volumes as forming a coherent whole. I am otherwise well aware that Vol. I is neither a text on analysis nor one on functional analysis. Any reader interested in a deeper understanding of such notions should consult the more standard texts referred to in Vol. I. Each volume is divided into consecutively numbered chapters. Chapter m contains an introduction, several sections numbered Sect. re.l, Sect. m.2, etc., and is concluded by a set of exercises. Within Sect. m.n, theorems are consecutively numbered, as Thin. re.n-l, Thm. m.n-2, etc., and figures are likewise consecutively numbered, as Fig. re.n-l, Fig. m.n-2, etc. Remarks and formulas are not numbered. The end of the proof of a theorem, or the end of a remark, is indicated by the symbol m in the right margin. In Chapter m, exercises are numbered as Ex. re.l, Ex. m.2, etc. All the important results are stated in the form of theorems (there are no lemmas, propositions, or corollaries), which therefore represent the core of the text. At the other extreme, the remarks are intended to point out some interpretations, extensions, counter-examples, relations with other results, that in principle can be skipped during a first reading; yet, they could be helpful for a better understanding of the material. When a term is defined, it is set in boldface if it is deemed important, or in italics otherwise. Terms that are only given a loose or intuitive meaning are put between quotation marks. Special attention has been given to the notation, which so often has a distractive and depressing effect in a first encounter with elasticity. In particular, each volume begins with special sections, which

viii

Mathematical Elasticity: General preface

the reader is urged to consult first, about the notations and the rules that have guided their choice. The same sections also review the main definitions and formulas that will be used throughout the text. Complete proofs are generally given. In particular, whenever a mathematical result is of particular significance in elasticity, its proof has been included. More standard mathematical prerequisites are presented (usually without proofs) in special starred sections, scattered according to the local needs. The proofs of some advanced, or more specialized, topics, are sometimes only sketched, in order to keep the length of each volume within reasonable limits; in this case, ad hoc references are always provided. These topics are assembled in special sections marked with the symbol b, usually at the end of a chapter. Exercises of varying difficulty are included at the end of each chapter. Some are straightforward applications of, or complements to, the text; others, which are more challenging, are usually provided with hints or references. This treatise would have never seen the light had I not had the good fortune of having met, and worked with, many exceptional students and colleagues, who helped me over the past three decades decipher the arcane subtleties of mathematical elasticity; their names are listed in the preface to each volume. To all of them, my heartfelt thanks! I am also particularly indebted to Arjen Sevenster, whose constant interest and understanding were an invaluable help in this seemingly endless enterprise! Last but not least, this treatise is dedicated to Jacques-Louis Lions, as an expression of my deep appreciation and gratitude.

August, 1986 and October, 1999

Philippe G. Ciarlet

PREFACE

TO VOLUME

11

A fascinating aspect of three-dimensional elasticity is that, in the course of its study, one naturally feels the need for studying basic mathematical techniques of matrix theory, analysis, and functional analysis; how could one find a better motivation? For instance: - Both common and uncommon results from matrix theory are often needed, such as the polar factorization theorem (Thm. 3.2-2), or the celebrated Rivlin-Ericksen representation theorem (Thm. 3.6-1). In the same spirit, who would think that the inequality [tr A B I < ~ i vi(A)vi(B), where vi(A) and vi(B) denote the singular values, arranged in increasing order, of the matrices A and B, arises naturally in the analysis of a wide class of actual stored energy functions? Incidentally, this seemingly innocuous inequality is not easy to prove (Thm. 3.2-4)! - The understanding of the "geometry of deformations" relies on a perhaps elementary, but "applicable", knowledge of differential geometry. For instance, my experience is that, among those of my students who had been previously exposed to modern differential geometry, very few could effectively produce the formula da~' = ICofVT~ nlda relating reference and deformed area elements (Thm. 1.7-1). - The study of geometrical properties (orientation-preserving character, injectivity) of mappings in IR3 naturally leads to using such basic tools as the invariance of domain theorem (Thms. 1.2-5 and 1.2-6) or the topological degree (Sect. 5.4); yet these are unfortunately all too often left out from standard analysis courses. - Differential calculus in Banach spaces is an indispensable tool which is used throughout this volume, and the unaccustomed reader should quickly become convinced of the many merits of the Frdchet derivative and of the implicit function theorem, which are the keystones to the existence theory developed in Chap. 6. - The fundamental Cauchy-Lipschitz ezistence theorem for ordinary differential equations in Banach spaces, as well as the conver1This "Preface to Volume I )' is an updated excerpt from the "Preface)' to the of Volume I.

K~st e d i t i o n ( 1 9 8 8 )

x

Preface to Volume I

gence of its approximation by Euler's method, are needed in the analysis of incremental methods, often used in the numerical approximation of the equations for nonlinearly elastic structures (Chap. 6). Basic topics from functional analysis and the calculus of variations, such as Sobolev spaces (which in elasticity are simply the "spaces of finite energy"), weak convergence, existence of minimizers for weakly lower semi-continuous functionals, pervade the treatment of existence results in three-dimensional elasticity (Chaps. 6 and 7). Key results about elliptic linear systems of partial differential equations, notably sufficient conditions for the W2'p(f~)-regularity of their solutions (Thm. 6.3-6), are needed preliminaries for the existence theory of Chap. 6. As a result of John Ball's seminal work in three-dimensional elasticity, convexity and the subtler polyconvezity play a particularly important rSle throughout this volume. In particular, we shall naturally be led to finding nontrivial examples of convex hulls, such as that of the set of all square matrices whose determinant is > 0 (Thm. 4.7-4), and of convex functions of matrices. For instance, functions such as F --~ ~i{)~i(FW-~)} a/2 with a > 1 naturally arise in the study of Ogden's materials in Chap. 4; while proving that such functions are convex is elementary for c~ = 2, it becomes surprisingly difficult for the other values of c~ >_ 1 (Sect. 4.9). Such functions are examples of John Ball's polyconvex stored energy functions, a concept of major importance in elasticity (Chaps. 4 and 7). - In Chap. 7, we shall come across the notion of compensated compactness. This technique, discovered and studied by Fran~;ois Murat and Luc Tartar, is now recognized as a powerful tool for studying nonlinear partial differential equations. -

-

-

Another fascinating aspect of three-dimensional elasticity is that it gives rise to a number of open problems, for instance: - The extension of the "local" analysis of Chap. 6 (existence theory, continuation of the solution as the forces increase, analysis of incremental methods) to genuine mixed displacement-traction problems; - "Filling the gap" between the existence results based on the implicit function theorem (Chap. 6) and the existence results based on the minimization of the energy (Chap. 7); An analysis of the nonuniqueness of solutions (cf. the examples given in Sect. 5.8); -

Preface to Volume I

xi

A mathematical analysis of contact with friction (contact, or self-contact, without friction is studied in Chaps. 5 and 7); -

- Finding reasonable conditions under which the minimizers of the energy (Chap. 7) are solutions of the associated Euler-Lagrange equations; While substantial progress has been made in the study of statics (which is all that I consider here), the analysis of time-dependent elasticity is still at an early stage. Deep results have been recently obtained for one space variable, but formidable difficulties stand in the way of further progress in this area. -

This volume will have fulfilled its purposes if the above messages have been conveyed to its readers, that is, if it has convinced its more application-minded readers, such as continuum mechanicists, engineers, "applied" mathematicians, that mathematical analysis is an indispensable tool for a genuine understanding of three-dimensional elasticity, whether it be for its modeling or for its analysis, essentially because more and more emphasis is put on the nonlinearities (e.g., injectivity of deformations, polyconvexity, nonuniqueness of solutions, etc.), whose consideration requires, even at the onset~ some degree of mathematical sophistication; -

if it has convinced its more mathematically oriented readers that three-dimensional elasticity~ far from being a dusty classical field, is on the contrary a prodigious source of challenging open problems. -

Although more than 570 items are listed in the bibliography, there has been no attempt to compile an exhaustive list of references. The interested readers should look at the extensive bibliography covering the years 1678-1965 in the treatise of Truesdell & Noll [1965], at the additional references found in the books by Marsden & Hughes [1983], Hanyga [1985], Oden [1986], and especially Antman [1995], and in the papers of Antman [1983] and Truesdell [1983], which give short and illuminating historical perspectives on the interplay between elasticity and analysis. The readers of this volume are strongly advised to complement the material given here by consulting a few other books, and in this respect~ I particularly recommend the following general references on three-dimensional elasticity (general references on lower-dimensional theories of plates, shells and rods are given in Vols. II and III):

xii

Preface to Volume I

In-depth perspectives in continuum mechanics in general, and in elasticity in particular: The treatises of Truesdell & Toupin [1960] and Truesdell & Noll [1965], and the books by Germain [1972], Gurtin [1981b], Eringen [1962], and Truesdell [1991]. - Classical and modern expositions of elasticity: Love [1927], Murnaghan [1951], Timoshenko [1951], Novozhilov [1953], Sokolnikoff [1956], Novozhilov [1961], Landau & Lifchitz [1967], Green & Zerna [1968], Stoker [1968], Green & Adkins [1970], Knops & Payne [1971], Duvaut & Lions [1972], Fichera [1972a, 1972b], Gurtin [1972], Wang & Truesdell [1973], Villaggio [1977], Gurtin [19Sla], Ne~as & Hlav&~ek [1981], and Ogden [1984]. Mathematically oriented treatments in nonlinear elasticity: Marsden & Hughes [1983], Hanyga [1985], Oden [1986], and the landmark book of Antman [1995]. - The comprehensive survey of numerical methods in nonlinear three-dimensional elasticity of Le Tallec [1994]. -

-

In my description of continuum mechanics and elasticity, I have only singled out two azioms: The stress principle of Euler and Cauchy (Sect. 2.2) and the axiom of material frame-indifference (Sect. 3.3), thus considering that all the other notions are a priori given. The reader interested in a more axiomatic treatment of the basic concepts, such as frame of reference, body, reference configuration, mass, forces, material frame-indifference, isotropy, should consult the treatise of Truesdell & Noll [1965], the books of Wang & Truesdell [1973] and Truesdell [1991], and the fundamental contributions of Noll [1959, 1966, 1972, 1973, 1978]. At the risk of raising the eyebrows of some of my readers, and at the expense of various abus de Iangage, I have also ignored in this volume the difference between second-order tensors and matrices. The readers disturbed by this approach should look at the books of Abraham, Marsden & Ratiu [1983] and, especially, of Marsden & Hughes [1983], where they will find all the tensorial and differential geometric aspects of elasticity explained in depth and put in their proper perspective. Likewise, Vol. III should be also helpful in this respect. This volume is an outgrowth of lectures on elasticity that I have given over the past 15 years at the Tata Institute of Fundamental Research: the University of Stuttgart, the Ecole Normale Sup~rieure,

Preface to Volume I

xiii

and the Universit4 Pierre et Marie Curie. I am particularly indebted to the many students and colleagues I worked with on that subject during the same period; in particular: Michel Bernadou, Dominique Blanchard, Jean-Louis Davet, Philippe Destuynder, Giuseppe Geymonat, Hu Jian-wei~ Srinivasan Kesavan, Klaus Kirchgiissner, Florian Laurent, Herv4 Le Dret, Jind~ich Ne~as, Robert Nzengwa, Jean-Claude Paumier, Peregrina Quintela-Estevez, Patrick Rabier, and Annie Raoult. Special thanks are also due to Stuart Antman, Irene Fonseca, Morton Gurtin, Patrick Le Tallec, Bernadette Miara~ Francois Murat, Tinsley Oden, and G4rard Tronel, who were kind enough to read early drafts of this volume and to suggest significant improvements. For their especially expert and diligent assistance as regards the material realization of this volume, I very sincerely thank H41~ne Bugler, Monique Damperat, and Liliane Ruprecht. August, 1986 and October, 1999

Philippe G. Ciarlet

This Page Intentionally Left Blank

PREFACE

TO VOLUME

II 1

Lower-dimensional plate, shell, and rod, theories that rely on a priori assumptions of a mechanical or geometrical nature have been proposed by A.-L. Cauchy, Sophie Germain, G. Kirchhoff~ T. yon Ks163 A.E.H. Love, E. Reissner~ Jakob Bernoulli, C.-L.-M.-H. Navier, L. Euler, S.-D. Poisson, E. and F. Cosserat, L.H. Donnell, W. Fliigge, S.P. Timoshenko, V.V. Novozhilov, I.N. Vekua, A.E. Green, W.T. Koiter~ J.G. Simmonds~ P.M. Naghdi, and others. There are two reasons why these lower-dimensional theories are so often preferred to the three-dimensional theory that they are supposed to "replace" when the thickness, or the diameter of the crosssection, is "small enough". One reason is their simpler mathematical structure, which in turn generates a richer variety of results. For instance, the existence, regularity, or bifurcation, theories, and more generally the "global analysis", are by now on firm mathematical grounds for nonlinearly elastic rods (see Antman [1995] for a scholarly and comprehensive exposition) or for nonlinearly elastic yon K~rm~n plates (see Ciarlet & Rabier [1980]). By contrast, these theories of global analysis are still partly in their infancies for nonlinear three-dimensional elasticity (see Marsden & Hughes [1983] and Vol. I for comprehensive surveys): After the fundamental ideas set forth by Ball [1977], who was able to establish the existence of a minimizer of the energy for a wide class of realistic nonlinearly elastic materials, there indeed remain manifold challenging open problems; for instance, there is no known set of sufficient conditions guaranteeing that such a minimizer satisfies the equilibrium equations even in the weak sense of the principle of virtual work (another existence theory, based on the implicit function theorem~ does not share this drawback, but it is restricted to problems with smooth data and to special boundary conditions~ unrealistic in practice; see Vol. I and the comprehensive treatment of

V l nt [19ss]). 1A substantial portion of this preface is an excerpt from the "Introduction" in Ciarlet & Lods [1996b].

xvi

Preface to Volume II

Another virtue of lower-dimensional theories is their far better amenability to numerical computations. For instance, directly approximating the three-dimensional displacement field of a cooling tower seems out of reach at the present time, even in the linearly elastic realm: The existing codes use two-dimensional equations, such as those of W.T. Koiter; see Bernadou [1994] for a comprehensive account. Likewise, although substantial progress has recently been achieved for directly approximating the "three-dimensional" displacement field of a linearly elastic rectangular plate, current codes are almost invariably based on two-dimensional equations, such as those of the Kirchhoff-Love or Reissner-Mindlin theories, whose numerical approximation is by now on essentially safe theoretical grounds; see, e.g., Ciarlet [1978, 1991], Glowinski [1984], Hughes [1987], Robert & Thomas [1991], Brezzi & Fortin [1991], Brenner & Scott [1994], Destuynder &: Salaun [1996]. Be that as it may, the locking phenomenon~ and the proper handling of boundary layers, in the numerical approximation of twodimensional plate or shell equations still pose challenging problems; for plates, see notably Arnold [1981], Bathe & Brezzi [1985], Brezzi & Fortin [1986], Hughes & Franca [1988], Pitk~iranta [1988], Bathe, Brezzi & Fortin [1989], Arnold & Falk [1989, 1990, 1996], Brezzi, Fortin & Stenberg [1991], Arnold & Brezzi [1993], Lyly, Stenberg & Vihinen [1993], Chenais & Paumier [1994], Schwab [1994, 1996], Schwab & Suri [1994], Schwab & Wright [1995], Suri, Sabu~ka & Schwab [1995], Pitk~iranta & Suri [1996]. Lower-dimensional models being thus widely used, two essential, and in fact intimately related, questions arise: Given a 'flower-dimensional" elastic body, together with specific loadings and boundary conditions, how to choose between the mani]old lower-dimensional models that are available? For instance, given a linearly elastic shell, which theory should be preferred, among those of Koiter, Naghdi, Novozhilov, Budiansky-Sanders, etc.? This question is of paramount practical importance, for it makes no sense to devise accurate methods ]or approximating the solution of a "wrong" model! Consequently, before approximating the exact solution of a given lower-dimensional model, we should first know whether it is "close enough" to the exact solution of the three-dimensional model it is intended to approximate. This observation leads to the second question:

Preface to Volume H

xvii

How to mathematically justify in a rational fashion a lower-dimensional model from the three-dimensional model? This question has been answered through three different approaches (only scant references are given here to these approaches, as many additional ones are provided throughout the text). The first approach consists in directly estimating the difference between the three-dimensional solution and the solution of a given, i.e., "known in advance", lower-dimensional model (this difference makes sense once the three-dimensional solution is properly averaged or the lower-dimensional one is extended in some fashion to a three-dimensional field). For linearly elastic plates, the first such estimate seems to be due to Morgenstern [1959], who cleverly used the Hellinger-Reissner variational principle of the linear theory; see also Morgenstern & Szab6 [1961], Goldenveizer [1969], Nordgren [1971, 1972], Simmonds [1971a], Ladev~ze [1976, 1980], Shoiket [1976], and Kohn & Vogelius [1985]. This approach was likewise successfully applied to linearly elastic shells by Koiter [1970], Simmonds [1971b], and Koiter & Simmonds [1973]. The second approach, essentially due to Naghdi [1972] for plates and shells, consists in using a hierarchic method, whose governing principle is an a priori assumption that the admissible displacement fields are restricted to a specific form. For a plate (to fix ideas), such "test functions" are finite sums of products of unspecified functions of the in-plane variables times given linearly independent functions of the "transverse" variable. The functions of the in-plane variables are then determined by inserting these test functions into the threedimensional equations or into the three-dimensional energy, a process that leads to the solution of a finite number of two-dimensional boundary value problems. Increasing the number of linearly independent functions of the transverse variable thus yields a "hierarchy" of models, which may be deemed two-dimensional, as they are determined by solving two-dimensional problems. References to this approach are numerous. For plates, see notably Naghdi [1972], Destuynder [1980, Chap. 5], Miara [1989], Sabu~ka & Li [1991, 1992], Schwab [1994, 1995, 1996], Alessandrini, Arnold, Falk & Madureira [1999], and Madureira [1999]; for rods, see Antman

[1972],

bur

[ 992], M sca e.has

T abur

[ 992],

Figueiredo & Trabucho [1993], and Antman [1995]; for shallow shells, see Figueiredo & Trabucho [1992]; for a general analysis, see Antman [1976] and Antman & Marlow [1991]. See also the related "con-

xviii

Preface to Volume H

straint method", advocated by Podio-Guidugli [1989, 1990] for modeling plates and shells. These two approaches nevertheless rely on some a priori assumptions of a mechanical or geometrical nature, intended to account for the "smallness" of a geometrical parameter and intended to be more effective as this parameter approaches zero. Hence the need arises to mathematically justify these a priori assumptions, together with

the lower-dimensional theories they engender, directly from threedimensional elasticity. Otherwise, these assumptions and theories can be thought of as being "handed down by some higher power (a Hungarian wizard, say)", to quote Truesdell [1978]. This direct justification is achieved by the third approach, which consists in applying an asymptotic method. It has recently received considerable attention, as exemplified by the books of Destuynder [1986] and Ciarlet [1990] for plates; Le Dret [1991] for plates and beams (straight rods); Trabucho & Viafio [1996] for beams; and Ciarlet [1990], Le Dret [1991], Kozlov, Maz'ya & Movchan [1999] for multi-structures. In a formal asymptotic method, the three-dimensional solution (the displacement field and, in some cases, the stress field) is first "scaled" in an appropriate manner so as to be defined on a fixed domain, then expanded as a formal series expansion in terms of a "small" parameter e, which is the "dimensionless" half-thickness of a plate or a shell, or the "dimensionless" diameter of the cross-section of the rod. "Dimensionless" means that e measures the ratio between the thickness or diameter and some "characteristic" dimension. For a cooling tower, for instance, where common values for the average thickness and height are 0.3m and 150m, the ratio 2e is thus equal to 1/500. It is worthwhile to keep in mind this order of magnitude. The formal series expansion of the scaled three-dimensional solution is then inserted into the three-dimensional problem, and sufficiently many factors of the successive powers of ~ found in this fashion are equated to zero until the leading term of the expansion can be computed and, presumably, identified with the scaled solution of a known lower-dimensional problem. Such a method is "formal" in that the series is not expected to converge (as an infinite series in powers of e); in fact, the successive terms of the expansion, except the leading one, cannot usually satisfy the boundary conditions of the three-dimensional problem! This situation is typical of such singular perturbation problems; see in this respect the comprehensive

Preface to Volume H

xix

treatments given in Lions [1973] and Eckhaus [1979]. The fundamental contributions of Priedrichs & Dressler [1961] and Goldenveizer [1962, 1964] for plates, Rigolot [1972, 1976] for rods, Goldenveizer [1963, 1964] for shells, are among the first successful attempts to apply formal asymptotic methods in linearized elasticity. Some restrictions or a priori assumptions were, however, still needed. Another shortcoming is the lack of convergence theorems of the scaled three-dimensional solution to the leading term of its formal expansion as ~ --+ 0, essentially because the asymptotic method is applied in these works to the partial differential equations of the three-dimensional problem; in this case, convergence results usually rely on a maximum principle (see Eckhaus [1979]), which does not hold for the system of linearized three-dimensional elasticity. Ciarlet & Destuynder [1979a, 1979b] applied instead the formal asymptotic method to the variational, or weak, formulation of the three-dimensional boundary value problems of linearly and nonlinearly elastic plates. Without making any a priori assumption of a mechanical or geometrical nature, they justified in this fashion the linear and nonlinear KirchhofJ-Love plate theories (only the magnitudes of the components of the applied loads and of the Lam4 constants must behave as appropriate powers of the thickness, but, as shown in a systematic way by Miara [1994a, 1994b], such asymptotic behaviors are unavoidable). This approach was extended to yon Kdrmdn plates by Ciarlet [1980], to Marguerre-von Kdrmdn shallow shells by Ciarlet & Paumier [1986] and Busse [1997], to general nonlinear constitutive equations by Davet [1986], to nonlinearly elastic plates with varying thickness by Quintela-Estevez [1989], and to nonlinear elastodynamics by Raoult [1988] and Karwowski [1993]. By allowing a larger class of behaviors on the applied loads, Fox, Raoult & Simo [1993] were also able to justify in this fashion twodimensional nonlinear "planar membrane" and "planar flezural " theories that are valid for "large" deformations and frame-indifferent, in that they share the same invariances as the three-dimensional theory (while Miara [1994b] assumed at the outset that the nonlinear twodimensional models found by the formal asymptotic method have to reduce to the classical ones once linearized, this assumption was not made by Fox, Raoult & Simo [1993], who were thus able to consider other classes of behaviors).

xx

Preface to Volume H

The one-dimensional equations of a nonlinearly elastic beam (a beam is a straight rod) were likewise justified by Cimeti~re, Geymonat, Le Dret, Raoult & Tutek [1988] and Karwowski [1990]. Nonlinear beam theory has also been related to the three-dimensional theory by Mielke [1988, 1990], who justified St Venant's principle by a remarkable use of the center manifold theorem. Various classes of lower-dimensional equations modeling "shallow" or "arbitrarily curved" nonlinearly elastic rods have been similarly identified by Karwowski [1996a, 1996b]. The most noticeable virtue of the asymptotic method applied to the weak formulation of linear elasticity problems is its amenability to a rigorous asymptotic analysis, which shows that the threedimensional scaled solution converges in some Hilbert spaces (H 1 or L 2) to the leading term of the formal asymptotic expansion as the "small" parameter approaches zero. Such convergence theorems have been established by Destuynder [1980, 1981], CaiUerie [1980], Ciarlet g~ Kesavan [1981], Kohn gz Vogelius [1984, 1985, 1986], Raoult [1985], Blanchard & Francfort [1987], Paumier [1991], Cioranescu & Saint Jean Paulin [1995, 1999], Destuynder & Gruais [1995], Aganovi(3, Maru~iS-Paloka & Tutek [1995], Dauge gz Gruais [1996, 1998a, 1998b], Paumier & Raoult [1997], Aganovid, Jurak, Maru~id-Paloka & Tutek [1998], Dauge, Djurdjevic & RSssle [1998a, 1998b], Andreoiu [1999b], Dauge, Djurdjevic, Faou & RSssle [1999], Dauge, Gruais 8r RSssle [1999], Djurdjevic [1999], RSssle [1999a, 1999b], and RSssle, Bischoff, Wendland & Ramm [1999] for linearly elastic plates; Ciarlet g~ Miara [1992a] and Busse, Ciarlet gz Miara [1996] for linearly elastic shallow shells; Bermudez & Viafio [1984], Aganovi~ & Tutek [1986], Geymonat, Krasucki & Marigo [1987], Trabucho & Viafio [1987], Raoult [1988], Veiga [1995], and Le Dret [1995] for linearly elastic beams (see also the comprehensive survey of Trabucho gc Viafio [1996] and the works cited therein). Special mention must also be made of the approach of Mielke [1995], who keeps the thickness fixed, but lets the lateral boundary of the plate "go away to infinity". In these works, the proofs essentially rely on the ideas and methods described and developed in Lions [1973] for analyzing "abstract" linear variational problems that contain a small parameter. Convergence theorems can also be obtained from F-convergence theory, as in Bourquin, Ciarlet, Geymonat g~ Raoult [1992] and Anzellotti, Baldo g~ Percivale [1994] for linearly elastic plates. A remarkable feature of F-convergence theory is that it also led to the

Preface to Volume H

xx2

first convergence result for planar nonlinearly elastic bodies, due to Le Dret & Raoult [1995a] who themselves based their approach on that of Acerbi, Buttazzo & Percivale [1991] for strings. After the earlier formal attempts of A.L. Goldenveizer cited supra, a first major step for linearly elastic shells was achieved by Destuynder [1980] in his doctoral dissertation (see also Destuynder [1985]), where a convergence theorem for membrane shells was "almost proved"; another major step was achieved by Sanchez-Palencia [1990], who clearly delineated the kinds of geometries of the middle surface and boundary conditions that yield either two-dimensional membrane, or two-dimensional flezural, equations when the method of formal asymptotic expansions is applied to the variational equations of three-dimensional linearized elasticity (see also Caillerie & SanchezPalencia [1995b] and Miara & Sanchez-Palencia [1996]). Then Ciarlet & Lods [1996b, 1996d] and Ciarlet, Lods & Miara [1996] carried out an asymptotic analysis of linearly elastic shells that covers all possible cases: Under three distinct sets of assumptions on the geometry of the middle surface, the boundary conditions, and the order of magnitude of the applied forces, they established convergence theorems in H 1, in L 2, or in ad hoc completion spaces, that justify either the linear two-dimensional equations of an "elliptic membrane shell", or those of a "generalized membrane shell", or those of a "flezural shell". Combining these convergences with results of Destuynder [1985] and Sanchez-Palencia [1989a, 1989b, 1992] (see also Sanchez-Hubert & Sanchez-Palencia [1997]), Ciarlet & Lods [1996c] have also justified the well-known two-dimensional Koiter equations of a linearly elastic shell (Koiter [1970]), again in all possible cases. For nonlinearly elastic shells, a first noteworthy achievement is due to John [1965, 1971], who showed that, in the absence of surface loads and "away from the edge", the state of stress is "approximately planar" and the stresses "parallel to the middle surface" vary "approximately linearly" across the thickness if the thickness is sufficiently small. These remarkable results laid the ground for the two-dimensional, linear and nonlinear, shell theories of Koiter [1966, 1970] and Koiter & Simmonds [1973]. However, in spite of their elegance and depth, John's results hold only for special cases of loadings; besides, they do not provide information "up to the boundary" (of the middle surface of the shell), let alone about the boundary conditions of the associated two-dimensional problem.

xxii

Preface to Volume H

What is especially remarkable in John's analysis (based on exceedingly delicate a priori estimates) is that the constitutive equation is of the most general form. His results were therefore the first indication that general stress-strain laws could also be successfully handled by an asymptotic analysis. Formal asymptotic methods can be applied to nonlinearly elastic shells as well. In this direction, the earlier attempts of Green [1962] and Green & Naghdi [1965], also described in Green & Zerna [1968, Chap. 16]~ are particularly worthy of interest. A major step was then achieved by Miara [1998] and Lods & Miara [1998], who showed in this fashion that the leading term of the asymptotic expansion of the scaled three-dimensional displacement~ again in terms of the thickness as the "small" parameter~ can be identified with the solution of nonlinear two-dimensional "membrane", or "flexural", shell equations, according to the geometry of the middle surface and the boundary conditions as in the linear case. See also Rao [1994] for spherical shells. Another approach has been proposed by Ge, Kruse & Marsden [1996] for justifying time-dependent, nonlinear Cosserat shell theories. Based on the Hamiltonian structure of the equations of threedimensional nonlinear elastodynamics, this approach combines the features of both the hierarchic and asymptotic methods; see also Kirchg/issner & Djurdjevic [1997]. Another major step is due to Le Dret & Raoult [1996], who established the first convergence theorem for nonlinearly elastic shells. To this ends they used r-convergence theory for justifying a nonlinear "membrane" shell model (which coincides with that obtained by Miara [1998] only for specific classes of deformations). Linear and nonlinear shell theories constitute the themes of Volume III. The objective of this volume is to show how asymptotic methods, with the thickness as the "small" parameter~ indeed provide a powerful means of justifying two-dimensional plate theories. More specifically~ without any recourse to any a priori assumptions of a geometrical or mechanical nature, it is shown in the linear case that the three-dimensional displacements~ once properly scaled, converge in H i towards a limit that satisfies the well-known twodimensional equations of the linear Kirchhoff-Love theory; the convergence of the stresses is also established.

Preface to Volume H

xxiii

In the nonlinear case, again after ad hoc scalings have been performed, it is shown that the leading term of a formal asymptotic expansion of the three-dimensional solution satisfies well-known twodimensional equations, such as those of the nonlinear Kirchhoff-Love theory, or the yon Kdrmdn equations. Special attention is also given to the first convergence result obtained by Le Dret & Raoult [1995a] in this case, which leads to two-dimensional large deformation, ~ameindifferent, nonlinear planar membrane theories. It is also shown that asymptotic methods can likewise be used for justifying other "lower-dimensional" theories, some known, some new, such as the two-dimensional equations of elastic shallow shells, and the coupled "pluri-dimensionar' equations of elastic multi-structures, i.e., structures with junctions. In each case, the existence, uniqueness or multiplicity, and regularity of solutions to the "limit" equations obtained in this fashion are also studied. Although I have chosen here the viewpoint of asymptotic methods, I have simultaneously tried to provide reasonable introductions, and references, to other approaches, such as the Reissner-Mindlin theory, Naghdi's theory, hierarchic plate theories, theories derived by the constraint method, etc. Fortunately, there remains an abundance of challenging open problems; for instance: -

Finding a rigorous justification of the Reissner-Mindlin equa-

tions; - Justification of the nonlinear Kirchhoff-Love theory by a convergence theorem as the thickness approaches zero; Existence of solutions of three-dimensional nonlinear plate problems obtained through a proper extension of the two-dimensional solutions (known to exist); -

- Existence theory for two-dimensional plate equations, without any restrictions on the boundary conditions or on the magnitude of the applied forces; Numerical comparison (essentially lacking at the present time, even in the linear case) between three-dimensional and two-dimensional solutions of plate equations; etc. -

xxiv

Preface to Volume H

For the reader's convenience, this volume is written in such a way that, to a large extent, each chapter can be read independently of the others" For instance, a devotee of the yon Ks equations may proceed directly to Chap. 5, without having necessarily mastered Chaps. 1 to 4, although I obviously do not wish that this always be the case! To this end, each chapter begins with a substantial introduction detailing the scalings and assumptions on the data, and expounding the main ideas and results. A reader in a hurry may thus get a quick idea of the content of this volume by reading the introductions of the five chapters; consulting the preliminary sections titled "Plate equations at a glance" and "Shallow shell equations at a glance" should also be helpful in this respect. As in Vol. I, I have tried to provide a "reasonably complete" bibliography, but in view of the formidable existing literature on plates, I am also well aware that the appended list of references is far from being exhaustive. I apologize for any significant reference that I may have inadvertently overlooked. This volume is an outgrowth of series of lectures that I have given during the past twenty years at Tel Aviv University, Fudan University, the University of Stuttgart, the University of Bucharest, the Ecole Polytechnique F6d6rale de Lausanne, Neresheim (Seminar der Deutschen Mathematiker-Vereinigung), the EidgenSssische Technische Hochschule (Ziirich), the Chinese University of Hong Kong, and the Universit6 Pierre et Marie Curie. Substantial portions of the manuscript were also completed during stays at many other places, notably at New York University (Courant Institute of Mathematical Sciences), Cornell University (Mathematical Sciences Institute), Brown University, the Istituto Mauro Picone (Roma), the University of Texas at Austin, Kyoto University, Stanford University, the Universidade de Santiago de Compostela, and the Istituto di Analisi Numerica (Pavia). I am in this respect particularly indebted to my hosts in all these institutions, as their kind hospitality greatly contributed to the completion of this enterprise! The support of the project "Junctions in Elastic Multi-Structures" of the European Cooperation "S.C.LE.N.C.E." Programme is also gratefully acknowledged. This volume is also an updated, completely re-organized, and considerably expanded version (about twice as long) of my earlier

Preface to Volume H

xxv

monograph "Plates and Junctions in Elastic Multi-Structures: An Asymptotic Analysis"~ co-published in 1990 by Masson, Paris, and Springer-Verlag, Berlin. These lecture notes were based on a course taught over the years at the Universit4 Pierre et Marie Curie, Paris, as part of our Doctoral School "D.E.A. d'Analyse Num4rique". This volume is for the most part the result of joint efforts. I am deeply indebted in this respect to Philippe Destuynder~ Herr6 Le Dret, Patrick Rabier, and Annie Raoult, whose fundamental contributions and kind cooperations were essential to the success of this enterprise. I am also very grateful to the many other students and colleagues who either collaborated with me on, or brought their own contributions to, the theory of plates: Martial Aufranc, Michel Bernadou, Dominique Blanchard, Fr6d4ric Bourquin, Monique Dauge, Jean-Louis Davet, Giuseppe Geymonat, Isabelle Gruais, Fr4d6ric d'Hennezel, Srinivasan Kesavan, Christophe Lebeltel, Bernadette Miara, Robert Nzengwa, Paula Oliveira, Jean-Claude Paumier, Peregrina QuintelaEstevez, Jos6 M. Rodr/guez, Luis Trabucho de Campos, Juan M. Viafio Rey, Xiang Yan. Special thanks are also due to Daniel Coutand, Karine Genevey, Herr6 Le Dret, Cristinel Mardare, Bernadette Miara, Arnaud Montenay, V6ronique Lods, and Sebastian Slicaru, who were kind enough to read preliminary versions of the manuscript and to propose many improvements. I express my particular appreciation to Stuart Antman for the manifold "grammatically elastic" advices he provided me with over the years; he is in particular responsible for suggesting the convenient terminologies "nonlinearly elastic" and "linearly elastic" that I so often use. I also thank Genevieve Raugel and Alice Traynard, who kindly translated for me the seminal article of yon Ks163 [1910]. A reproduction of p. 350 of this article, where the celebrated "yon Kgrm~n equations" appeared for the first time in print, is shown on page lxiii. Last but not least, I express my heartfelt gratitude to Mathieu Ciarlet, who greatly helped me through the arduous task of compiling the bibliography. January, 1997 and October, 1999

Philippe G. Ciarlet

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PREFACE

TO VOLUME

III 1

The objective of this volume is to lay down the proper mathematical foundations of the two-dimensional theory of shells. To this end, it provides, without any recourse to any a priori assumptions of a geometrical or mechanical nature, a mathematical justification of two-dimensional nonlinear and linear shell theories, by means of asymptotic methods, with the thickness as the "small" parameter. A major virtue of this approach is that it naturally leads to precise mathematical definitions of "membrane" and "flezural" shells, be they nonlinearly or linearly elastic. Another noteworthy feature is that it automatically provides in each case the "limit" two-dimensional energy, together with the function space over which it should be minimized. This process highlights in particular the rSle played by two fundamental tensors, each associated with a displacement field of the middle surface, the change of metric and change of curvature tensots (either in eztenso in the nonlinear theories, or in their linearized version in the linear theories). More specifically, under fundamentally distinct sets of assumptions bearing on the geometry of the middle sur]ace, on the boundary conditions, and on the order of magnitude o] the applied forces, it is shown t h a t in the linear case, the three-dimensional displacements, once properly scaled, converge (in H I, or in L 2, or in ad hoc completions) towards a "two-dimensional" limit that satisfies either the

linear two-dimensional equations of a "membrane" shell (themselves divided into two subclasses) or the linear two-dimensional equations

of a "flezural" shell. Under the same assumptions, the two-dimensional linear Koiter equations are also justified for all the above classes of linearly elastic shells. The existence and uniqueness of solutions to each of these linear 1The preceding "Preface to Volume Ir' should be read in conjunction with the present one, since most of its content is as relevant to shell theory as it is to plate theory.

xxviii

Preface to Volume III

equations are also studied in detail, essentially by means of crucial inequalities of Korn's type on surfaces. In the nonlinear case, again under fundamentally distinct sets of assumptions on the geometry of the middle surface, on the boundary conditions, and on the order of magnitude of the applied forces, it is shown that the leading term of a formal asymptotic expansion of the three-dimensional solutions, once properly scaled, satisfies either the nonlinear two-dimensional equations o] a "membrane" shell, or the nonlinear two-dimensional equations of a "flexural" shell. Another class of two-dimensional equations for a nonlinearly elastic "membrane" shelly this time justified by means of a convergence theorem, is also discussed. Finally the existence of solutions to the "limit" nonlinear equations obtained in the above fashions is also studied. Thanks to the timely availability of S.S. Antman's admirable book "Nonlinear Problems of Elasticity" (Springer-Verlag, 1995), I do not dwell, however, on the approach that consists in "directly" viewing a shell as a two-dimensional deformable body, in the spirit of the Cosserat shell theories. Fortunately, there remains an abundance of challenging open problems; for instance: A justification, by a convergence theorem as the thickness approaches zero, of the nonlinear membrane and flexural theories obtained by a formal method in Chaps. 8 to 10; - A clarification of the respective applicabilities of the two nonlinear membrane shell theories described in Chap. 9; A higher-order asymptotic analysis, including error estimates, for linearly elatic shells (such an analysis has been successfully developed for linearly elastic plates; cf. Vol. II, Sect. 1.12); A "local" theory of shells, accounting for the possible coexistence of regions with a "membrane-dominated" behavior with ones with a "flexural-dominated" behavior (as the theory presented in this volume is a "limit" one, it gives rise to a single, "global", behavior); - An analysis of singularities "away from the boundary" (i.e., other than boundary layers) that appear in some "generalized membrane" shells; - An asymptotic justification of Naghdi's shell equations; A refined classification of nonlinearly elastic shells (the definitions proposed in this volume still do not account for some examples -

-

-

-

Preface to Volume III

xxix

and do not seem to be entirely coherent with the definitions of the linear theory; see the commentaries in Sects. 9.1 and 10.2); A numerical comparison between three- and two-dimensional solutions, so as to test the "range of validity" (in terms of data) of the limit two-dimensional equations; etc. -

Naturally, this volume relies heavily on elementary notions from differential geometry in I~3. However, I do not assume any a priori knowledge of this subject, whose needed prerequesites are expounded at length in the first two chapters. This volume is thus entirely selfcontained in this respect. Be that as it may, this volume is neither a treatise on differential geometry nor one on tensor analysis: The incursions into these fields have been kept to the minimum required here (for instance, the definitions of a "tensor" is nowhere to be found in this volume). In the same spirit, I have consistently given explicit, but occasionally lenghty, formulas rather than more condensed, intrinsic, ones. This patti pris may irritate some differential geometers or shell aficionados, but it should render the book more accessible to browsers and non-experts; for the same reason, I have systematically avoided using the (otherwise quite convenient!) terminology "immersion". At the expense of intentional repetitions, most chapters are written in such a way that they are as sel]-contained as possible. I apologize to those readers, brave enough to read the entire volume, who might be annoyed by such a procedure. As in Vol. II, each chapter begins with a substantial introduction expounding its main results. A reader in a hurry may thus get a quick idea of the contents of this volume by reading the introductions of the eleven chapters. Consulting the preliminary sections titled "Twodimensional linear shell equations at a glance" and "Two-dimensional nonlinear shell equations at a glance" should also be helpful in this respect. I have tried to provide a "reasonably complete" bibliography about "mathematical" shell theory (only scant incursions are otherwise provided into the engineering or computationally-oriented literature), but I am also well aware that the appended list of references is far from being exhaustive: Shell theory has offered so many challenges during its long history that it has generated an immense literature.

xxx

Preface to Volume III

As a complement, I advise the readers of this volume to consult great classics, such as Fliigge [1934], Pogorelov [1956, 1966, 1967], Vlasov [1958], Novozhilov [1959, 1970], Goldenveizer [1961], Mushtari

a C limo [ 961],

a

[1968], Timo he o

Womow ky-

Krieger [1970], Fliigge [1973], Rutten [1973], as well as more recent treatments, such as Vinson [1974], Pietraszkiewicz [1977, 1979], Lukasiewicz [1979], Dikmen [1982], Calladine [1983], Sasar & Kr~itzig [1985], Niordson [1985], Vekua [1986], Axelrad [1987], Gould [1987], Pogorelov [1988], Destuynder [1990], Dym [1990], Sernadou [1994], Antman [1995], Stolarski, Selytschko & Lee [1995], Valid [1995], Sanchez-Hubert & Sanchez-Palencia [1997], Libai & Simmonds [1998], Vorovich [1999]. I also recommend the short, but illuminating, accounts by Sanchez-Palencia [1995] and Chapelle & Bathe [1998a] of the often elusive behavior of shells and of the difficulties inherent in their finite element analysis. Substantial portions of the manuscript were completed during stays at the Romanian Academy (Bucharest), the University of Bucharest, the Istituto di Analisi Numerica (Pavia), Fudan University, the University of Stuttgart, and the Liu Bie-ju Centre for Mathematical Sciences of the City University of Hong Kong. I am deeply indebted to my hosts in these institutions: Viorel Barbu, Marius Iosifescu, George Dinc~, Franco Brezzi, Li Ta-tsien, Klaus Kirchg~ssnet, and Roderick Wong. In particular, the first three chapters are an outgrowth of a series of lectures that I delivered at the University of Stuttgart, thanks to the Alexander yon Humboldt-Stiftung, whose support is gratefully acknowledged. These lectures, which greatly beneficiated from the critical comments of Mariana Haragus-Courcelle, Ivica Djurdjevie, and Andreas RSssle, later became a monograph "Introduction to Linear Shell Theory", co-published in 1998 by Gauthier-Villars, Paris and North-Holland, Amsterdam; cf. Ciarlet [1998c]. The support of the project "Shells: Mathematical Modeling and Analysis, Scientific Computing" by the "Human Capital and Mobility" Programme of the Commission of the European Communities is also gratefully acknowledged. This project culminated in an "International Conference on Shells", organized with the highest maestria by Juan Manuel Viafio in Santiago de Compostela in 1997. I also wish to express my deep appreciation to the far-sightedness of those who created the Institut Universitaire de France. Without

Preface to Volume III

xxxi

this remarkable institution, the writing of this volume would have required several additional years! This volume is for the most part the result of joint efforts. I am deeply indebted in this respect to Michel Bernadou, Philippe Destuynder, Herv~ Le Dret, V~ronique Lods, Cristinel Mardare, Bernadette Miara, Annie Raoult, and Evariste Sanchez-Palencia, whose fundamental contributions and kind cooperations were essential to the success of this enterprise. I am very grateful to the many other students or colleagues who also contributed in some way to the content of this volume: Georgiana Andreoiu, Adel Blouza, St~phane Busse, Denis Caillerie, Ma'it~ Carrive, Dominique Chapelle, Christophe Collard, Daniel Coutand, Monique Dauge, Isabel de Figueiredo, Karine Genevey, Giuseppe Geymonat, Patrick Giroud, Liliana Gratie, Oana Iosifescu, Srinivasan Kesavan, Fran~;ois Larsonneur, Patrick Le Tallec, Arnaud Montenay, Jean-Claude Paumier, Paolo Podio-Guidugli, Olivier Ramos, Rao Bopeng, Anne Roquefort, Sebastian Slicaru, Xiao Li-ming. Special thanks are also due to Elena Baderko, Adel Blouza, Dominique Chapelle, Daniel Coutand, Liliana Gratie, Herv~ Le Dret (in particular, for stimulating discussions about the nonlinear membrane theories!), Cristinel Mardare, Qin Tie-hu, Anne Roquefort, and Karim Trabelsi, who kindly read preliminary versions of the manuscript and suggested many improvements. I renew my particular appreciation for Stuart Antman, whose kind semantic assistance has been an invaluable help over so many years. October 1999

Philippe G. Ciarlet

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TABLE OF CONTENTS'

Mathematical Elasticity: General plan

...........

ii

......... v Preface t o Volume I . . . . . . . . . . . . . . . . . . . . . . . ix xv Preface t o Volume I1 . . . . . . . . . . . . . . . . . . . . . . xxvii Preface t o Volume 111. . . . . . . . . . . . . . . . . . . . . Differential geometry at a glance . . . . . . . . . . . . . . xxxix Mathematical Elasticity: General preface

Three-dimensional elasticity in curvilinear coordinates at a glance . . . . . . . . . . . . . . . . . . . . . . . xlvii Two-dimensional linear shell equations at a glance

...

li

.

lvii

Two-dimensional nonlinear shell equations at a glance

PART A.

LINEAR SHELL THEORY

Chapter 1. Three-dimensional linearized elasticity and Korn's inequalities in curvilinear coordinates Introduction . . . . . . . . . . . . . . . . . . . . . . . 1.1. Three-dimensional linearized elasticity in Cartesian coordinates . . . . . . . . . . . . . . . . . . . . . . . . 1.2. Curvilinear coordinates and metric tensor in a threedimensional domain . . . . . . . . . . . . . . . . . . . 1.3. The variational equations of three-dimensional linearized elasticity in curvilinear coordinates . . . . . . . 1.4. Covariant derivatives and Christoffel symbols in a threedimensional domain . . . . . . . . . . . . . . . . . . . 1.5. Linearized change of metric tensor in curvilinear coordinates . . . . . . . . . . . . . . . . . . . . . . . . . 1.6. The boundary value problem of three-dimensionallinearized elasticity in curvilinear coordinates . . . . . .

'

3 3

5 12

22 32 35 37

'The symbol indicates a section where most results are stated without proof.

xxxiv 1.7.

Table of contents

A l e m m a of J. L. Lions; t h r e e - d i m e n s i o n a l K o r n ' s inequalities a n d infinitesimal rigid d i s p l a c e m e n t l e m m a in curvilinear coordinates . . . . . . . . . . . . . . . .

40

Existence a n d uniqueness t h e o r e m in curvilinear coordinates . . . . . . . . . . . . . . . . . . . . . . . . .

50

1.9 ~. Complement" Recovery of a t h r e e - d i m e n s i o n a l manifold from its metric tensor field . . . . . . . . . . . . .

54

1.8.

Exercises

Chapter

. . . . . . . . . . . . . . . . . . . . . . . . .

2. I n e q u a l i t i e s o f K o r n ' s t y p e o n s u r f a c e s Introduction

. . .

.......................

56 61 61

2.1.

Curvilinear coordinates a n d metric tensor on a surface

63

2.2.

C u r v a t u r e tensor on a surface

73

2.3.

Covariant derivatives a n d Christoffel s y m b o l s on a surface . . . . . . . . . . . . . . . . . . . . . . . . . .

85

2.4.

Linearized change of metric tensor on a surface . . . .

90

2.5.

Linearized change of c u r v a t u r e tensor on a surface . .

93

2.6.

Inequalities of K o r n ' s t y p e a n d infinitesimal rigid disp l a c e m e n t l e m m a on a general surface . . . . . . . . .

100

I n e q u a l i t y of K o r n ' s t y p e a n d infinitesimal rigid disp l a c e m e n t l e m m a on an elliptic surface . . . . . . . .

117

2.8 ~. C o m p l e m e n t - Recovery of a surface from its m e t r i c a n d c u r v a t u r e tensor fields . . . . . . . . . . . . . . .

130

2.7.

Exercises

Chapter

. . . . . . . . . . . . . . . . . . . . . . . . .

132

3. A s y m p t o t i c a n a l y s i s o f l i n e a r l y e l a s t i c s h e l l s : Preliminaries and outline ............ 137 Introduction

3.1.

.............

.......................

T h e t h r e e - d i m e n s i o n a l e q u a t i o n s of a linearly elastic shell . . . . . . . . . . . . . . . . . . . . . . . . . . . .

137 141

3.2.

T h e t h r e e - d i m e n s i o n a l equations over a d o m a i n independent ofe .......................

149

3.3.

G e o m e t r i c a l a n d mechanical preliminaries . . . . . . .

154

3.4.

T h e t w o - d i m e n s i o n a l equations of linearly elastic " m e m b r a n e " a n d "flexural" shells derived by m e a n s of a f o r m a l a s y m p t o t i c analysis . . . . . . . . . . . . . . . 161

3.5.

S u m m a r y of the convergence t h e o r e m s . . . . . . . . .

183

Exercises

190

. . . . . . . . . . . . . . . . . . . . . . . . .

xxxv

Table of contents

Chapter 4. Linearly elastic elliptic membrane shells Introduction

. . 193

.......................

193

4.1.

L i n e a r l y elastic elliptic m e m b r a n e shells: Definition, example, a n d a s s u m p t i o n s on the data; the threed i m e n s i o n a l e q u a t i o n s over a d o m a i n i n d e p e n d e n t ofr . . . . . . . . . . . . . . . . . . . . . . . . . . . .

4.2.

Averages w i t h respect to the t r a n s v e r s e variable

4.3.

A t h r e e - d i m e n s i o n a l inequality of K o r n ' s t y p e for a family of linearly elastic elliptic m e m b r a n e shells . . . 205

4.4.

C o n v e r g e n c e of the scaled displacements as r --4 0

4.5.

T h e t w o - d i m e n s i o n a l e q u a t i o n s of a linearly elastic elliptic m e m b r a n e shell; existence, uniqueness, a n d regu l a r i t y of solutions; f o r m u l a t i o n as a b o u n d a r y value problem . . . . . . . . . . . . . . . . . . . . . . . . . .

223

J u s t i f i c a t i o n of the t w o - d i m e n s i o n a l e q u a t i o n s of a linearly elastic elliptic m e m b r a n e shell; c o m m e n t a r y a n d refinements . . . . . . . . . . . . . . . . . . . . . . . .

230

Exercises

. . . . . . . . . . . . . . . . . . . . . . . . .

235

Chapter 5. Linearly elastic generalized membrane shells . . . . . . . . . . . . . . . . . . . . . . . . .

241

4.6.

5.1.

196

. . . 201

. . 209

Introduction ....................... 241 L i n e a r l y elastic generalized m e m b r a n e shells: Definition a n d a s s u m p t i o n s on the data; the t h r e e - d i m e n s i o n a l e q u a t i o n s over a d o m a i n i n d e p e n d e n t of r . . . . . . . 245

5.2.

A n a l y t i c a l preliminaries . . . . . . . . . . . . . . . . .

248

5.3.

A t h r e e - d i m e n s i o n a l inequality of K o r n ' s t y p e for a family of linearly elastic shells . . . . . . . . . . . . .

258

G e n e r a l i z e d m e m b r a n e shells of the first a n d second kinds . . . . . . . . . . . . . . . . . . . . . . . . . . .

261

A d m i s s i b l e applied forces . . . . . . . . . . . . . . . .

264

5.4. 5.5. 5.6.

C o n v e r g e n c e of the scaled displacements as ~ --~ 0

5.7.

T h e t w o - d i m e n s i o n a l e q u a t i o n s of a linearly elastic generalized m e m b r a n e shell; existence a n d u n i q u e n e s s of solutions . . . . . . . . . . . . . . . . . . . . . . . .

287

J u s t i f i c a t i o n of the t w o - d i m e n s i o n a l e q u a t i o n s of a linearly elastic generalized m e m b r a n e shell; examples, c o m m e n t a r y , a n d refinements . . . . . . . . . . . . . .

291

Exercises

297

5.8.

. . . . . . . . . . . . . . . . . . . . . . . . .

. . 266

xxxvi

Table of contents

Chapter 6. Linearly elastic flexural shells . . . . . . . . . Introduction

299

.......................

299

6.1.

Linearly elastic flexural shells: Definition, examples, a n d a s s u m p t i o n s on the data; the t h r e e - d i m e n s i o n a l equations over a d o m a i n i n d e p e n d e n t of ~ . . . . . . .

6.2.

Convergence of the scaled displacements as ~ --~ 0

6.3.

T h e two-dimensional equations of a linearly elastic flexural shell; existence a n d uniqueness of solutions . 317

6.4.

Justification of the two-dimensional equations of a linearly elastic flexural shell; c o m m e n t a r y a n d refinements . . . . . . . . . . . . . . . . . . . . . . . . . . .

323

Exercises

328

302

. . 308

.........................

Chapter 7. Koiter's equations and other two-dlmensional linear shell theories . . . . . . . . . . . . . . . . 333 Introduction 7.1.

7.2. 7.3.

.......................

333

T h e two-dimensional Koiter equations for a linearly elastic shell: Existence, uniqueness, a n d r e g u l a r i t y of solutions; formulation as a b o u n d a r y value p r o b l e m . 335 Justification of Koiter's equations for all types of linearly elastic shells . . . . . . . . . . . . . . . . . . . . 345 Koiter's equations: Additional c o m m e n t a r y a n d bibliographical notes . . . . . . . . . . . . . . . . . . . .

360

7.4.

T h e two-dimensional N a g h d i equations for a linearly elastic shell; existence a n d uniqueness of solutions . . 363

7.5.

O t h e r linear shell theories . . . . . . . . . . . . . . . .

367

7.6.

Linear shallow shell theories

369

Exercises

PART

B.

..............

.........................

NONLINEAR

SHELL

372

THEORY

Chapter 8. A s y m p t o t i c a n a l y s i s o f nonlinearly elastic shells: Preliminaries . . . . . . . . . . . . . . . . . . . . 381 Introduction 8.1. 8.2.

.......................

381

T h r e e - d i m e n s i o n a l nonlinear elasticity in C a r t e s i a n coordinates . . . . . . . . . . . . . . . . . . . . . . . . .

386

T h r e e - d i m e n s i o n a l nonlinear elasticity in curvilinear coordinates . . . . . . . . . . . . . . . . . . . . . . . .

392

Table of contents

8.3.

xxxvii

T h e three-dimensional equations of a nonlinearly elastic shell . . . . . . . . . . . . . . . . . . . . . . . . . .

403

T h e three-dimensional equations over a d o m a i n indep e n d e n t of s . . . . . . . . . . . . . . . . . . . . . . .

407

G e o m e t r i c a l a n d mechanical preliminaries . . . . . . .

411

8.6.

T h e m e t h o d of formal a s y m p t o t i c expansions . . . . .

413

8.7.

T h e leading t e r m is of order zero . . . . . . . . . . . .

415

8.8.

Identification of a two-dimensional variational problem satisfied by the leading t e r m . . . . . . . . . . . .

424

Exercises

.........................

430

Chapter 9. Nonlinearly elastic membrane shells . . . . .

433

8.4. 8.5.

Introduction 9.1. 9.2.

.......................

433

Nonlinearly elastic m e m b r a n e shells: Definition, examples, a n d a s s u m p t i o n s on the d a t a . . . . . . . . .

436

T h e two-dimensional equations as a variational problem . . . . . . . . . . . . . . . . . . . . . . . . . . . .

443

9.3.

T h e two-dimensional equations as a m i n i m i z a t i o n problem . . . . . . . . . . . . . . . . . . . . . . . . . . . . 445

9.4.

T h e two-dimensional equations of a nonlinearly elastic m e m b r a n e shell derived by means of a formal asymptotic analysis; c o m m e n t a r y . . . . . . . . . . . . . . .

447

9.5 b. T h e two-dimensional equations of a nonlinearly elastic m e m b r a n e shell derived by means of r - c o n v e r g e n c e theory; c o m m e n t a r y . . . . . . . . . . . . . . . . . . .

453

Exercises

.........................

465

Chapter 10. Nonlinearly elastic flexural shells . . . . . .

469

Introduction

.......................

469

10.1. Identification of a two-dimensional variational problem satisfied by the leading t e r m when there are nonzero admissible inextensional displacements . . . . . . . . 472 10.2. Nonlinearly elastic flexural shells: Definition, examples, a n d a s s u m p t i o n s on the d a t a . . . . . . . . . . .

502

10.3. T h e two-dimensional equations as a variational problem . . . . . . . . . . . . . . . . . . . . . . . . . . . .

507

10.4. T h e two-dimensional equations as a m i n i m i z a t i o n problem . . . . . . . . . . . . . . . . . . . . . . . . . . . . 519

Table of contents

xxxviii

10.5. T h e t w o - d i m e n s i o n a l e q u a t i o n s o f a n o n l i n e a r l y e l a s t i c f l e x u r a l shell d e r i v e d b y m e a n s o f a f o r m a l a s y m p t o t i c analysis; c o m m e n t a r y

. . . . . . . . . . . . . . . . . .

521

10.6. E x i s t e n c e o f s o l u t i o n s to t h e m i n i m i z a t i o n p r o b l e m

. 526

Exercises

. . . . . . . . . . . . . . . . . . . . . . . . .

539

C h a p t e r 11. Koiter's equations and other t w o - d i m e n s i o n a l nonlinear shell theories . . . . . . . . . . . . . 545 Introduction

. . . . . . . . . . . . . . . . . . . . . . .

545

11.1. T h e t w o - d i m e n s i o n a l K o i t e r e q u a t i o n s for a n o n l i n -. . . . . . . . . . . . . . . . .

545

11.2. O t h e r n o n l i n e a r shell t h e o r i e s . . . . . . . . . . . . . .

e a r l y elastic shell . . . .

549

11.3. N o n l i n e a r s h a l l o w shell t h e o r i e s

552

References Index

............

. . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

557 583

DIFFERENTIAL

1. 2. 3. 4.

GEOMETRY

AT A GLANCE

~

General conventions Differential geometry of three-dimensional domains in IR3 Differential geometry of surfaces in R 3 Korn's and other inequalities in curvilinear coordinates

I. G E N E R A L

CONVENTIONS

(i) Latin indices and exponents: i, j, p, . . . , take their values in the set {1, 2, 3}, unless otherwise indicated as when they are used for indexing sequences. (ii) Greek indices and exponents: c~, ~, or,... , except s and u in the outer n o r m a l derivative operator 0~, take their values in the set {1, 2). (iii) T h e repeated index summation convention is systematically used in conjunction with conventions (i) and (ii). (iv) T h e symbol %" designates a p a r a m e t e r t h a t is > 0 and approaches zero.

2. D I F F E R E N T I A L GEOMETRY OF THREE-DIMENSIONAL DOMAINS

I N IR8

a . b: Euclidean inner product of a C ]~3 and b E IR3. a A b: exterior p r o d u c t of a E IR3 and b C IR3. la I: Euclidean n o r m of a E IR3. iOnly the notations and definitions that are specific to shell theory are listed in this section and the next ones, which otherwise complement the section "Main notation, definitions, and formulas" in Vol. I.

xl

Differential geometry at a glance

f~: domain in R z (open, bounded, connected subset of R z with a Lipschitz-continuous boundary, the set f~ being locally on one side of its boundary). x - (mi)" generic point in f~. din" volume element in f~. 0 Ozi F" boundary of f~. dr" area element along r . (ni)" along r .

unit outer normal vector (defined dP-almost everywhere)

(9 9~ C I~3 --+ R z" injective and smooth enough mapping such that the three vectors 0il!i)(m) are linearly independent at each point mEf~. gi = OiO" vectors of the covariant bases in the set (9(f~); this means that, at each x E f~, the three vectors gi(m) - 0 i O ( z ) form the covariant basis at the point (9(x). 9 i" vectors of the contravariant bases in the set (9(~); the vectors 9i(m) are defined at each m E ~ by the relations gi(m) 99j(m) - 6j. covariant components of the metric tensor of the set

g i j -- O i ' O j "

g -- det(gij). gij _ g i . g j , set O(f~).

contravariant components of the metric tensor of the

r ip = gP. Ojgi: Christoffel symbols. Villi -- Ojvi - - ~ i jPV p . 9 covariant derivatives of a vector field r i g i with covariant components vi " f~ -+ IR. oiJ Ilk - Ok crij + Fpko'PJ + P{q ~

covariant derivatives of a tensor .

.

field with contravariant components a zJ 9fl ~ I~. g o ( v ) " covariant components of the metric tensor of the set (o + k eillj(V) -- 1Cgij(V ) - gij] lin : 1

89

" g i + Oiv " g j ) P

9covariant components of the linearized change of metric tensor associated with a =

( ,llJ +

Jll,) -

+

-

Differential geometry at a glance

xli

displacement field ~ - - r i g i of the set | the notation [.-.]tin denotes the linear part with respect to v in [... ]. E Ijj(

) -

- g j)

__

1

-- ~(Vill/+ Villi + gmnvmlliVnllj ) . covariant components of the change of metric tensor, also called the Green-St Venant strain tensor, associated with a displacement field rig i of the set (!i)(~).

3.

DIFFERENTIAL

GEOMETRY

OF

SURFACES

IN

R3

w: domain in I~2 (open, bounded, connected subset with a Lipschitz-continuous boundary, the set w being locally on one side of its boundary). y-

(ya)" generic point in ~.

dy" area element in w. 0 02 - ~, 0~ 0,~ Oy,~ OyaOy~ 7: boundary of the set w. dT: length element along 7. (va): unit outer normal vector along 7. (7"a) with

T 1 --" - - V 2 ,

T 2 --" V l :

unit tangent vector along 7.

Or8 -- vaOaS: outer normal derivative of 8 along 7. 0~-8 -- 7"aOaS: tangential derivative of 8 along 7. 8 9~ C R 2 -+ R 3" injective and smooth enough mapping such that the two vectors OaS(y) are linearly independent at each point yE~. S - 8(~): surface. vectors of the covariant bases of the tangent planes; this means that, at each y E ~, the two vectors OaS(y) form the covariant basis of the plane tangent to S at the point 8(y) E S. aa

-

OaS:

aa: vectors of the contravariant bases of the tangent planes; at each y E ~, the vectors aa(y) of the plane tangent to S at 8(y) are defined by the relations aa(y) 9a~(y) - ~ . a3

--a

3 =

al

Aa2

xlii

Differential geometry at a glance

covariant components of the metric tensor of the

aa~ = a a . a o : surface S.

a = det (aao). a a13 - -

a a.

a ~"

contravariant components of the metric tensor

of S. bao - a 3" O~aa" covariant components of the curvature tensor of S. b~a - aOabaa: mixed components of the curvature tensor of S. F~ 71al~

- a ~ . O~aa" Christoffel symbols. -

-

O ~ r l a - F ~ r / ~ and ~31~ -- O~r/3: covariant derivatives of a

vector field yia / with covariant components r/i : ~ -+ JR. yal~ - 0 ~ a + r ~ r / ~ , covariant derivatives of a tangential vector field ~ T a a a with contravariant components r/a : ~ -+ ]R. flail ~ - - rlal~ -- ba~rl3

and ~311t3- r/31~ - b~r/~.

rla~l~ - O~n a~ + r~nZ" + r{~n ~ . covariant derivatives of a tensor field with contravariant components n a ~ 9 ~ JR.

~1~ -

0~

+ r~bX - r ~ .

co~i~=t derivatives of the

curvature tensor, defined here by means of its mixed components ~ 9~ - + ]R. aa~(r/): covariant components of the metric tensor of the surface

(o + ,7~a~)(~). -~,~(,) - 89[ a ~ ( n ) - aa~] "'~ -- 89(0~,) 9a,~ + 0 ~ 0 " a ~ ) -- ~-(~o1~ + ~ , ~ ~)89 covariant components of the linearized change of metric tensor associated with a displacement field ~ - y i a ' of the surface S; the notation [... ]tin denotes the linear part with respect to r~ in [... ].

~(~)

-

89

. a~ + o~

.

~).

bat,(r/): covariant components of the curvature tensor of the surface (0 + yia')(-~) (only defined at those points in U where the two vectors Oa(O + ~7iai) are linearly independent).

~(~)

-

[ b ~ z ( . ) - b~Z] ~" - (O~Z# - r x ~ o ~ )

9a3

= ~ I ~ - b ~ b ~ + b ~ l ~ + b;~,~ + b ; l ~ = 0~.~

-

r ~ 0~ ~

-

b,~ ~,,.~,7~

+~g(0~.~ - r;~.~) + b;(O~ +(0~b; + r~b~

- r~.~)

- r a~b~)~Tr ~ " covariant components of

Differential geometry at a glance

xliii

the linearized change of curvature tensor associated with a displacement field ~ - rlia i of the surface S; the notation [... Izin denotes the linear part with respect to r / i n [..-]. ~(0)

-

(0~

- r~o~O)

. as.

1 G a ~ ( r l ) - -1~ ( a a ~ ( u ) - - a a ~ ) - ~(rla lf3 +rl~l a +amnrimll,arlnl ~), w h e r e a mn = a m 9an: covariant components of the change of metric tensor associated with a displacement field ~Tiai of the surface S.

Raf~ (r/) - baf~(r/) - baf~" covariant components of the change of metric tensor associated with a displacement field rlia i of the surface S (only defined if the two vectors Oa(O+rlia i) are linearly independent in w).

4. K O R N ' S A N D O T H E R I N E Q U A L I T I E S CURVILINEAR COORDINATES 1

IN

Given a domain a in R n, the norm in L~(a) or 1,2(fl) is noted 10,a and the norm in Hm(fl) or Hm(fl), m >_ 1, is noted II" I[m,a. T h r e e - d i m e n s i o n a l Korn's inequality "without boundary conditions" in curvilinear coordinates (Thm. 1.7-2):

i

i,j

for a11 v - ( v i ) E Hl(f~). T h r e e - d i m e n s i o n a l Korn's inequality in curvilinear coordinates (Thm.

1.7-4): }1/2 IlVlll, a 0,

A ~ j k t _ )~gij gkt + D(gik gfl + git gjh), and # are the Lam~ constants of the constituting elastic material, g - det(gij), the functions fi C L2(12) and h i E L2(rl), where r l -- 0 ~ - r0, account for the applied body and surface forces, and the linearized strains in curvilinear coordinates eillj(v) E L2(~) are defined for each v - (vi) e H I ( ~ ) by 1

ei[Ij(V ) -- ~(OjVi + OiVj) - Fijvp, p P -- gP " Oigj. where Fij

The interest of this calculation is that it naturally introduces essential notions, such as the covariant derivatives vijlj - - O j V i - - rijV of a vector field rig i and the linearized change of metric tensor associated with this vector field, found here by means of its covariant components 1

~llJ(~) - ~(~llJ + ~Jlli).

These notions are then studied in greater details for their own sake (Sects. 1.4 and 1.5). We also describe in detail (Thm. 1.6-1) the equivalent boundary value problem when it is likewise expressed in terms of curvilinear coordinates. Finally, we show how a fundamental lemma of J.L. Lions (Thm. 1.7-1) can be put to use for directly establishing Korn's inequality in

Linearized elasticity in Cartesian coordinates

Sect. 1.1]

5

curvilinear coordinates: This inequality, which asserts the existence of a constant C such that (Thm. 1.7-4)

}1/2

Ilvlll, n 0 is given. The surface S is defined as S = O(~), where w C R 2 and 0 : ~ ---> E s is a smooth injective mapping. Each point $" of { ~ ' } - is thus of the form ~" - | z2, z~) - O(zx, zn) + z ~ a 3 ( z l , z~.), where as(z1, z2) is a unit vector normal to S at the point 8(Zl, z2) and (zl , ~2, ~ ) E ~" = ~ x [-~, el. For e > 0 small enough, the mapping @ : = ~ • [-e, e] is also injective and the curvilinear coordinates of any point $~ E {fl~} - are then defined as the coordinates of the unique point ~ - (Xl, z~., ~ ) E ~ such that $~ = |

mapping.

Let a3 denote a continuously

varying unit normal

a l o n g S', a n d let

~.-

~•

~, ~[.

vector

14

Three-dimensional linearized elasticity

[Ch. 1

Hence the set ( ~ e } - is given by

-

e

where the mapping O 9~e C I~s --+ E 3 is defined by

(~) ($gl, X2, ;gl):: O(;gl, Lg2)-{-xla3(xl, ;g2) for aU (Xl, x2, x~) E ~ . If the mapping @ 9~ E 3 is injective (as is the case if ~ > 0 is small enough; cf. T h m . 3.1-1), each point ~e _ ( ~ , xl, x~) e { ~ e } is the image &e _ | of a unique point x e - (xl, x2, x~) e ~ , the three coordinates xl~ x2~ x~ of which are called the ~ n a t u r a P ~ e u r v i l i n e a r c o o r d i n a t e s of $~.

Remark. Later on, the curvilinear coordinates xa will be denoted Ya~ so as to afford the short notation y for a generic point in ~. m If a linearly elastic shell is subjected to applied forces and to a b o u n d a r y condition of place, the displacement field inside {~e } - satisfies the equations of three-dimensional linearized elasticity in Cartesian coordinates described in Sect. 1.1. As we shall see t h r o u g h o u t this volume, it turns out that an essential preliminary to the asymptotic analysis of such a shell problem when e approaches zero consists in rewriting these equations in terms of the curvilinear coordinates xl, x2, x~ (the "new" variables) instead of the Cartesian coordinates x~, xl, xl (the "old" variables). As a preparation to this rewriting~ we review in this section basic definitions and properties of curvilinear coordinates in a "general" three-dimensional domain ~ C Ea; thus the exponents e have no longer any raison d'etre. Let there be given a three-dimensional affine Euclidean space E a, a Cartesian frame i n E a a n d a d o m a i n ~ C ~a as in Sect 1.1 In addition, let there be given a three-dimensional vector space in which three vectors e i - ei form a basis; this space will accordingly be identified with I~3. We let xi denote the coordinates of a point x in this space and we let Oi := O/Oxi and Oij := 02/OxiOxi. Assume that there exist a domain ~ in I~3 and an injective mapping O 9 ~ -+ E a such that O ( ~ ) - { ~ } - . Hence each point

Sect. 1.2]

~ 3 ~.

Curvilinear coordinates and metric tensor

.,....

,,.*

~'.

e~.~.........'.'.'.'.'.': ....i""

15

-.. .....

e

Fig. 1.2-2: Curvilinear coordinates and domain. T h e three coordinates z l , z2, zs of $ - | G {(1}-. W h e n e v e r t h e y are g~(z) -- 0 i | form the covariant basis t h e coordinate lines passing t h r o u g h ~.

covariant bases in a three-dimensional of z E 12 are the curvilinear coordinates linearly independent, the three vectors at $ -- | t h e y are t h e n t a n g e n t to

& E {l~}- can be unambiguously written as

-

O(z),

x c 12,

and the three coordinates Xi of x are called the c u r v i l i n e a r c o o r d i n a t e s of ~ (Fig. 1.2-2). Naturally, there are infinitely many ways of defining curvilinear coordinates in a given domain ~, depending on how the domain 12 and the mapping O are chosen! Examples of curvilinear coordinates include the well-known cylindrical and spherical coordinates (see Fig. 1.2-3 and also Ex. 1.1). Another instance is provided by the curvilinear coordinates xl, x2, x~ used for defining a shell (Fig. 1.2-1); note that, in this instance, each set of curvilinear coordinates ~1, x2 on the surface S gives rise to a set of curvilinear coordinates in {l~e} -. Assume that the mapping O - | i 9~ C R s ~ {l~}- C g 3 is differentiable at a point x E 12. If ~z is such that (~ + 6 z ) C 12, we

Three-dimensional linearized elasticity

16

[Ch. 1

!

Fig. 1.2-3" Two familiar ezamples of curvilinear coordinates. Let 1~ be a threedimensional domain. The cylindrical coordinates of $ E ~ are ~o, p, z. The spherical coordinates of $ E ~ are ~o, ~, r. Special care must of course be exercised in order that such eurvilinear coordinates be unambiguously defined, since the same point is defined by (~o, p, z), or (~o + 2k~r, p, z), or (~o + k~r, - p , z), k E Z; in addition, neither ~o nor ~ are defined at the origin r As is customary, these coordinates are appended directly to the set 1"~, but they are in fact coordinates in a different domain f~, not represented here!

thus have

e(~ + ~ ) - e ( ~ ) + v e ( ~ ) o ~ + o ( ~ ) , w h e r e t h e m a t r i x V O ( x ) is g i v e n b y

VO(x):=

/

0t| 02Or 03

~t

0102 0202 0302 0t| 0203 0303

(x).

L e t t h e t h r e e v e c t o r s g i ( x ) C IR3 b e d e f i n e d b y

g~(~) .- o , |

/Oi@l/

[0,02 \o~03

(~),

Sect. 1.2]

Curvilinear coordinates and metric tensor

17

so t h a t gi(x) is the i-th column vector of the matriz V O ( ~ ) . Let ~ e = fi~iei; then the expansion of ~9 about ~ may also be written as

e(~ + 0~) = e ( ~ ) + 0~a~(~) + o ( ~ ) . If in particular ~ z is of the form ~a~ = ~tei, where ~t E Ii~ and e i is one of the basis vectors in I~s, this relation reduces to

e ( ~ + ~t~) = e ( ~ ) + ~tg~(~) + o(~). We henceforth assume that the three v e c t o r s gi(X) are linearly independent, in which case they constitute the e o v a r i a n t b a s i s at the point ~ - O(x). The last relation thus shows that, in this case, each vector gi(x) is tangent to the i-th c o o r d i n a t e line passing through - O(x), defined as the image by {9 of the points of ~ that lie on the line parallel to ei passing through x; cf. Fig. 1.2-2 (there exist to and tl with to < tl and 0 E [to, tl] such that the equation of the i-th coordinate line is t E [to, tl] --+ fi(t) : - O ( x + tei) in a sufficiently small neighborhood of ~; hence f~(0) - Oi| - gi(x)). Naturally, we are committing here a convenient abus de langage: The vector tangent to the i-th coordinate line at $ = | is in fact t h a t vector in the affine space E 3 that is parallel to gi(x) and has as its origin. R e t u r n i n g to a general increment ~ e = ~xiei, we also infer from the expansion of O about x that (recall that we use the s u m m a t i o n convention)"

te(~ + ~)-

e(~)l 2 - ~ T v e ( ~ ) T v e ( ~ ) ~

+ o (16~12)

In other words, the principal part of the length between the points | + ~z)and | {~xigi(x) 9gi(x)~xJ}l/2. This observation suggests the introduction of the symmetric matriz (gij (x)) of order three, whose elements

Three-dimensional linearized elasticity

18

[Ch. 1

are the c o v a r i a n t c o m p o n e n t s of the m e t r i c t e n s o r at ~ - O(x). Note that the matrix V O ( x ) is invertible and that the matrix (gij(x)) is positive definite, since the vectors gi(x) are assumed to be linearly independent. A w o r d of c a u t i o n . We refrain here from following the common, but improper, usage of calling "metric tensor" the matrix (gij(x)) itself. In spite of its convenience, it is a confusing and flagrant abus de langage, for the "genuine" metric tensor also has "contravariant components" gij (x) (see the next theorem); it even has "mixed comi ponents" gj(x) (which are simply the Kronecker symbols ~ ) . See, e.g., Antman [1996, Chap. 11]. II In the next theorem, we review fundamental formulas showing how volume, area, and length elements at a point a~ = O(x) in the set { ~ } - can be expressed either in terms of the matrix V O ( x ) or in terms of the matrix (gij(x)) or of its inverse matrix (gii (x)); see also Fig. 1.2-4. Parts (a) and (b) win be immediately put to use in the next section; part (c) provides the essence of the metric tensor. Otherwise, we refer to Vol. I, Sects. 1.5 to 1.8, for comments and references. If A is a square matrix, C o f A denotes the cofactor matrix of A. If A is invertible, we thus have C o f A - (det A ) A -T (details about the cofactor matrix may be found in Vol. I, Sect. 1.1). Also note that the assumptions made on the mapping O guarantee that { ~ } - - O ( ~ ) and that the boundaries F of l~ and r of ft are related by F - O(F) (Vol. I, Thin. 1.2-8 and Ex. 1.7). T h e o r e m 1 2 - 1 Let f~ be a domain in R 3 let | "-~--+ E 3 be an injective and smooth enough mapping such that the three vectors gi(x) := OiO(x) are linearly independent at all points x e f~, and let -

(a) The volume element d$ at ~, - O(x) E ~ is given in terms of the volume element dx at x E f~ by d~ - [det V O ( x ) [ dz - v / g ( x ) d x ,

where g(X) : : det(gij(x)) and gii(x)"= g i ( x ) , gj(x).

Curvilinear coordinates and metric tensor

Sect. 1.2]

19

)

f2

,g~

a?..+

fi: \

I .......

E

Fig. 1.2-4: Volume, area, and length elements in curvilinear coordinates. The elements d~, d r ( S ) , and di($) at $ = | E {1~}- are expressed in terms of dz, d r ( z ) , and 6~ at z E II by means of the covariant and contravariant components of the metric tensor; el. Thin. 1.2-1. The corresponding relations are used for computing the volume of a subdomain ~r = O(V) C { h } - , the area of a surface A = | C 0 ~ , and the length of a curve C = | C { ~ } - , where C - :f(I) and I C R.

( b ) The area e l e m e n t d r ( ~ ) at ~ -

|

E O h is given in t e r m s

of the area e l e m e n t d F ( z ) at z E Of~ by

d~(~) - ICofVO(x)n(x)l dr(x)

where n ( z ) ' - n i ( z ) e

i denotes the u n i t outer n o r m a l vector at z E Of~,

20

Three-dimensional linearized elasticity

[Ch. 1

and the matrix (gij(x)) is the inverse of the matrix (gij(x))"

, ~

The components g '3 (x) of this matrix are called the contravariant c o m p o n e n t s o] the m e t r i c tensor a t x .

(r The te,~gth ele,~,~t di(~) ~t ~ - 0 (~) e { h } - i, gi~,~ by

~[(~)- { ~ v o ( ~ ) ~ v o ( ~ ) ~ } ~ / ~ -

- {~%(~)~J}~/~,

where $o~ = (~xiei . Proof. The relation d~ = [ det V | dx between the volume elements is well known. The relation g(x) = [det ~70(x)[ 2 follows from the relation (gij(x)) V(~)(x)Tv~)(X). Indications about the proof of the relation between the area elements dF(&) and dr(x) given in (b) are found in Vol. I, Thin. 1.7-1 (naturaUy, n(x) - ni(x)e i is identified here with the column vector in ]Ra with ni(x) as its components). Using the relations C o f ( A T) - ( C o f A ) T and C o f ( X B ) - ( C o f A ) ( C o f B ) , we next have: -

-

[CofVO(x)n(x)] 2 - n(x)TCof (VO(x)Tvo(x))n(x) . .

= g(~)~(~)g'~(~)~(~). Either expression of the length element given in (c) simply recalls that dl($) is by definition the "principal part" with respect to Sa~ of the length 1(9(x + Sa~) - O(x)[, whose expression precisely led to the introduction of the matrix (gij (x)). m The relations found in Thm. 1.2-1 are used for computing volume integrals, areas, and lengths inside {~}-" Let V be a subdomain of ~, let V "- O(V), and let ] " V --+ ~ be a d&-measurable function. Then

Sect. 1.2]

In particular, the

Curvilinear coordinates and metric tensor

21

volume of V is given by

Next, let A C 0fl be a surface, let 2{ := O(A) C 0~, and let ]z" 2{ -+ IR be a dr-measurable function. Then

fA h(&) dF(&) - fA In particular, the

(h o O)(x)v/g(x)~//ni(x)giJ(x)nj(x) dr(x).

area of 2{ is given by

a~a A "- f:~dF(&) = / A

v/g(x) ~/ni(x)giJ (x)nj(x) dF(x).

Finally, consider a curve C - f(I) in ~, where I is a compact interval of I~ and if - j:Zei 9I -+ ~ is a smooth enough injective mapping. Then the length of the curve C := O(C) C { ~ } - is given by

length C "-- f / [-~ d (0 o f)(t)l dt

~g

d/i

df j (t) dr. (t)-~

Let (f~ be yet another way of designating the Kronecker symbol. Given a point x E f~, the nine relations i

unambiguously define three linearly independent vectors gi(x), which form the e o n t r a v a r i a n t basis at the point ~ = O(x). To see this, let ~ p~io~i g ' ( ~ ) -

xik(~)gk(~)

i . the ~ e l ~ t i o . s g ~ ( ~ ) . 0 ~ ( ~ ) -

~j.

xik(x)gkj(x) = 5j; consequently, xik(x) = gik(x), where (gij(x)) "- (gij(x)) -1 (Thm. 1.2-1 (b)). This also shows that

This gives

= g~k(~)gj~(~)gk~(~ ) _ g ~ k ( ~ ) ~

_ g~j(~),

22

[Ch. 1

Three-dimensional linearized elasticity

and thus the vectors gi(x) are linearly independent since the matrix (g~J(x)) is positive definite. We would likewise establish that g~(~) - g~j(~)gJ(~). Let us record for convenience these fundamental relations between the vectors of the covariant and contravariant bases and the covariant and contravariant components of the metric tensor: gij(X) -- g i ( x ) "

gj(x)

and

gij (z)

- g i ( z ) 9gJ (z),

gi(~) - gij(~)g j(~) ~nd g~(~) - g~J(~)gj(~). In Sect. 1.9, we shall briefly discuss the reciprocal question of

recovering a three-dimensional manifold 0(~) from its metric tensor field: Given a positive definite symmetric matrix field (gij) on ~, find conditions under which there exists a mapping O : ~ --~ E 3 such that

OiO . OjlD = gij

in f~.

Indications about the meaning of the adjectives "covariant" and "contravariant" used in the definitions of the components of the metric tensor are provided in Ex. 1.3. Otherwise they can be simply seen as particularly effective (though possibly mysterious!) definitions. 1.3.

THE VARIATIONAL EQUATIONS OF THREE-DIMENSIONAL LINEARIZED ELASTICITY IN CURVILINEAR COORDINATES

Our point of departure is the variational formulation of the equations of three-dimensional linearized elasticity described in Sect. 1.1, which consist in finding fi = (ui) such that ~t e V ( h ) = {~ = (~3i) e H i ( h ) ; ~ = 0 Oil r 0 ) ,

ffi AiJkt~k,(it)~ij(~ ) d~ - f~ /igi d~ + ~1 hi~i d~ for all ~ - ( ~ i )

E V(h),

where ~ is a domain, with boundary r partitioned as r - F0 U r l ,

Sect. 1.3]

Variational equations in curvilinear coordinates

23

in the affine Euclidean space t; 3,

ft~jkl _ AS~jSkl + tt(Sik5 jl + 5ilSJ~),

a n d / i E L2(~) and hi e L 2 ( r l ) are given functions. These equations are expressed in terms of the Cartesian coordinates xi of the points & - (xi) C ( ~ ) - and of the Cartesian components ~ti, fz, h z of the displacement and force densities. As in Sect. 1.2, we assume that we are also given a domain ft, with b o u n d a r y F, in R 3 and a smooth enough injective mapping O 9 ~ --+ t; 3 such t h a t O ( ~ ) - { ~ ) - and the three vectors gi(x) - 0iO(x) are linearly independent at all points x E f~. Our objective consists in expressing these equations in terms of the curvilinear coordinates xi of the points & - O(x) E { ~ } - , where x - (xi) E f~. In other words, we wish to carry out a change of variables, from the "old" variables xi to the "new" variables xi, in each one of the integrals appearing in the above variational equations, which we thus wish to write as ^ .

^

~

/h...d~c-f...dx

f~l...dF-frl...dF,

and

where F1 C F and O (F1) -- F1. Because the "old" unknowns ~i 9 { ~ } - -+ I~ are the components of a vector field, some care must evidently be exercised in the definition of the "new" unknowns, which must be related to the old ones by means of an intrinsic quantity, i.e., having "physical invariance". Observing that the displacement vector ~i(~)&i at each point & E { ~ } - possesses this property, we define three new unknowns ui " gt --+ I~ by requiring that (Fig. 1.3-1)

~i(&).&i =: ui(x)gi(x) for all & - O(m), m e ~, where the three vectors gi(x) form the contravariant basis at ~ - O (x) (Sect. 1.2). Using the relations g i ( x ) . g j ( x ) - ~ and &i. &j _ 5~, we immediately find how the old and new unknowns are related, viz.,

-

-

24

Three-dimensional linearized elasticity

[Ch. 1

OCt.

Fig. 1.3-1: Three.dimensional elasticity in curvilinear coordinates. In curvilinear coordinates, the displacement vector "tl,i(~)gi(~,) of the point $ = | E (l is de-

fined by its covariant components ui(z) over the contravariant basis vectors gi (z) defined by gi(z).gj(z) = J~, where gj(z) = OjO(z). In Cartesian coordinates, the same displacement vector ~i($)~ i is defined by its Cartesian components fii($) over the vectors ~i of the Cartesian frame chosen in Es; cf. Fig. 1.1-1. Let

[gj(x)] i := g j ( x ) . &i a n d [gJ(x)]i ' - g J ( x ) " &i, i.e., [gj(x)] i denotes the i-th c o m p o n e n t of the vector g j ( x ) a n d [gJ(x)]i denotes the i-th c o m p o n e n t of the vector g J ( x ) over the basis {&l, ~2, &3} _ {&l, &2, &3} of the E u c l i d e a n space E 3 associated w i t h the affine space E3; cf. Sect. 1.1. In terms of these n o t a t i o n s , the preceding relations thus become

uj(x) - ~i(ir

i a n d ui(x) - uj(x)[g j (x)]i, $ - |

T h e three c o m p o n e n t s ui(x) are called the e o v a r i a n t c o m p o n e n t s of the d i s p l a c e m e n t v e c t o r a t ~, a n d the three functions

Sect. 1.3]

25

Variational equations in curvilinear coordinates

m

ui " ~ -+ IR defined in this fashion are called the c o v a r i a n t c o m p o n e n t s of the d i s p l a c e m e n t field uig i 9 -+ E s.

A w o r d of c a u t i o n . The "old" unknown/,(&) - (fii(&)) e IR3 could be justifiably identified with the displacement vector ~i(&)~ i itself since the space E 3 may be identified with the space IR3 once the basis {~1, ~2, ~3} is given in E 3. However, this is no longer true -

e e 3 , sinr

its

ompo.r

u i ( x ) now represent the components of the displacement field over the basis {gt(x), g2(x), g3(x)}, which varies with x e -ft. m m

We likewise associate "new" functions vi" fl --+ IR with the "old" functions ~)i 9{(~}- --+ IR appearing in the variational equations by letting ~i(~)& i - " va(x)ga(x) for all & - O(x), x e ~.

R e m a r k . As the functions 72i belong to the Sobolev space HI((~), they are in fact equivalence classes of functions, and any function in a class is in fact only defined almost everywhere. Accordingly, the relations defining the (equivalence classes of) functions ui (which likewise belong to the Sobolev space HI(fl) under ad hoc assumptions on the mapping O; cf. Thm. 1.3-1) need hold only for almost all E O(fl). But in order to avoid cumbersome statements, we blithely omit such mentions, m

We begin the change of variables by considering the integrals found in the right-hand side of the variational equations, i.e., those corresponding to the applied forces. With the Cartesian components ]i . (~ _ O ( ~ ) -+ IR of the applied body force density, let there be associated its c o n t r a v a r i a n t c o m p o n e n t s f i . fl _+ IR, defined by

/ i ( ~ ) e i --" f i ( x ) g i ( X ) for a11 ~ - O(x), x e fl. This definition shows that

and consequently that f i E L2(f~) if ]J C L2(~). It also implies that

Three-dimensional linearized elasticity

26

[Ch. 1

]i(x)~i(~ ) = (]i(~,)~i) . (~)j(X)eJ) :

for all & = |

]i(&)r

(fi(x)~i(X))"

(Vj(X)OJ(X)) : ]i(x)Vi(X)

x E f~. Hence

- fi(x)vi(x)v/g(xi dx for all ~ - O(x),x e f~,

since d& - v/g(x)dx (Thm. 1.2-1 (a)), and thus

f . fivi d& - / ~ fivi ~ dx.

Remarks. (1) What has just been proved is in effect the invariance of the number fi(x)vi(x) with respect to changes of curvilinear coordinates, provided one vector appears by means of its "contravariant" components (i.e., on the "covariant" basis) and the other by means of its "covariant" components (i.e., on the "contravariant" basis). Naturally, this number is nothing but the Euclidean inner product of the

two vectors! (2) The adjectives "covariant" and "contravariant" used in the definitions of the components of the displacement and force vector fields are given a proper interpretation in Ex. 1.2. II W i t h the Cartesian components h / 9 ~1 - O ( r l ) --+ R of the applied surface force density, let there be likewise associated its cont r a v a r i a n t c o m p o n e n t s h / . r l -~ ]~, defined by

hi(&)&idr(& ) -" hi(x)gi(x)v/g(x)dr(x) for all ~ - O(x), x C where the area elements d~(&) at & - | are related by (Thm. 1.2-1 (b))

e r l and d r ( x ) at x e r l

This definition shows that

for all ~ = |

x E rl,

Variational equations in curvilinear coordinates

Sect. 1.3]

hence that h i E

L~(r~) if h i

27

E L2(rl), since

hi(x) -- ~/nk(x)gkt(x)nt(x) hJ(F~)[gi(x)]j.

The factor {nkgmnt} -1/2 is introduced in the definition of the functions h i in order that

frl ~i~)idr - f r l hiviv/g dr,

i.e., in order that the same factor v/~ appears in both integrals fn fiviv/'g dx and fr~ hiviv/~ dr. It in turn gives rise to a more "natural" boundary condition on F1 when the variational equations are transformed into a boundary value problem (Thm. 1.6-1). Transforming the integrals appearing in the left-hand side of the variational equations seems to be a similarly innocuous enterprise, simply requiring in addition applications of the chain rule, since firstorder derivatives occur in the integrands. In fact, carrying out this transformation in a finite time is a subtle task, which relies in particular on the notion of covariant differentiation of a vector field; cf. part (iii) of the next proof. T h e o r e m 1.3-1. h~ e L ~ ( ~ ) b~ g i , ~ the weak solution of Cartesian coordinates

Let ~ be a domain in E 3, let ]i C L2(~) and Inactions, ~ d t~t ~ (~i) c V(fi) d ~ o t ~ the associated linearized elasticity problem in (Sect. 1.1).

Let ~2 be a domain in IRa and let O be a s of-~ onto { ~ } - - O ( ~ ) , so that the vectors gi(x) - OiO(x) are linearly independent at all points x E -~. Let the vectors g~(x) be defined by the relations g i ( x ) , gj(x) - 5j and let g(x) - det(gi(x ) 9gi(x)) and 9 ~j(~) - a~(~) 9a j(~), 9 e ~. Then the vector field u - (ui) "-~ -+ I~3 defined by

~ti(&)~ i =: ui(x)gi(x) for all & -- O(x), x 6 ~,

Three-dimensional linearized elasticity

28

[Ch. 1

satisfies the following variational problem: U e V(~):=

{~ --

(Vi) e

HI(~);

"v = 0 011 r 0 ) ,

fa A~Jk'ekll,(u)eill,(v)~/~dz - f y'v~/~ dz + fr h%~v~dr 1

fo~ all ~ = (~1 e v ( a ) ,

where ro . - o - l C P o ) , r l := o-l(:P1), the ]unctions h i E L 2 ( r l ) are defined by: ]i($)&i d$ : : v / g ( x ) f i ( x ) g i ( x ) d x ,

~- |

fi

x e f~,

hi(~)~i dr(~) =: v/g(~)hi(x)gi(x) dF(x), ~ - | the functions A ijkt - A jikt - A kui

AiJkl

:__

E cl(~)

L2(f~) and

e

x E rl,

are defined by:

Agijgkt + iz (gik gj! q_ gil gjk),

and finally, the functions eillj(v) - ejlli(~ ) E L2(~) are defined for all v E HI(~) by:

P eillj(v) := ~1 (0j,~ + 0 ~ j ) -rijvp, where

r~5 . - g~.O~gj : rj~i e c~

Proof. The following convention holds throughout this proof: The simultaneous appearance of ~ and x in an equality means that they are related by & = O(x) and that the equality in question holds either for all x E (2 or for almost all x E (2. (i) A,othe~ ~ , e ~ i o ,

of [g~(~)]k "- g~(~)" ek.

Let O(x) - | and (9(&) = Oi(~)ei, where 19" { ~ } - ~ _ denotes the inverse mapping of | Since O ( O ( x ) ) - x for all x e f~, the chain rule (see, e.g., Vol. I, Thm. 1.2-1) shows that the matrices

Sect. 1.3]

Variational equations in curvilinear coordinates

29

VO(x)

"-- (0jOk(:c)) (the row index is k) and ~ r 6 ( ~ ) : = (~k~)i(~)) (the row index is i) satisfy

vo(~)ve(~)

- ~,

or equivalently,

ojos(~) i = 5j.

The components of the above column vector being precisely those of the vector gj(x), the components of the above row vector must be those of the vector gi(x) since gi(x) is uniquely defined for each exponent i by the three relations g i ( x ) . g j ( r . ) - ~ , j - 1, 2, 3. Hence the k-th component of gi(x) over the basis {&l, e2, &3) has the following expression in terms of the inverse mapping {b"

[g~(~)]k - & ~ ( e ) . (ii) Definition of the Christoffel symbols. We next compute the derivatives Otgq(x) (the fields gq = gqrg r are of class C1 on ~ since O is assumed to be of class C2) as they will clearly be needed (see (iii)) for expressing the derivatives Oj~i(a~) as functions of x (recall that u i ( x ) - uk(x)[gk(x)]i). The vectors gk(x) forming a basis, we may write a priori

0~g~(~) - -r~k (~)gk (~), thereby unambiguously defining functions r~k 9~ -+ I~, Which are called the Christoffel symbols. To find their expressions in terms of the mappings O and ~), we observe that

r~(~) - r~(~)5~

- rT~(,)g~(,),

g~(~) - - 0 , g ~ ( ~ ) . g~(~),

and, noting that Ot(gq(x) 9gk(x)) -- 0 and [gq(X)]p - OpE)q(~), we obtain

rTk(~) - g~(~). 0~gk(~) - 8 ~ q ( ~ ) 0 ~ k o p ( ~ )

- r~,(,).

30

[Ch. 1

Three-dimensional linearized elasticity

Since O ~ C2(~;~ 3) and O e C~({fi}-; ~3) by assumption, the last relations show that r~t ~ C~ (iii) Let ~ -- (~)i) be given in the space V(~).

Then the vector field v - (vi) defined by ~)i(~)e i -- V i ( x ) g i ( x ) iS in the space V(f~); moreover,

~(~)

- ,kll~(~)[g~(~)]~[g~(~)]~,

where

~11~(~) . - o ~ ( ~ 1

- r~(~)~(~)

denotes a "covariant derivative" of the vector field vkg k at x, [gk(x)]i denotes the i-th component of gh(x) over the basis {&l, &2, &3), and r~k(x) - g q ( x ) . Orgy(x) are the Christoffel symbols introduced in (ii).

By a classical result about composite mappings (see, e.g., Ne~as [1967, Chap. 2, Lemma 3.2] or Adams [1975, Thm. 3.35]), a function o (9 is in H1(~2)if ~ e H I ( ~ ) a n d | ~ -+ { ~ } - - | a bijection such that both O and its inverse mapping O are Lipschitzcontinuous; consequently, the functions ~j o O are in H l(f~). Since the functions [gi]1 are in C1(~), the functions vi - (6j o O)[gi]J are thus in Hl(fl); besides, they satisfy vi - 0 on r0 since ~3j - 0 on r0. We next compute the partial derivatives vSj~3i(~) as functions of z by means of the relation ~3i(~) - Vk(X)[gk(x)]i 9 To this end, we first note that a differentiable function w" fl --+/~ satisfies

~j~(6(e)) - 0 ~ ( ~ ) ~ j ~ ( e ) -

o~(~)[g~(~)]~,

by the chain rule and by (i). In particular then,

= 0~k(~l[g~(~l]j[gk(~)]~ + ~(~1 (0~[g~(~)]i)[g~(~l]j :

(0~,~(~1 - r T ~ ( ~ ) , ~ ( ~ ) ) [ g k ( x ) ] i [ g l ( x ) ] j ,

since O t g q ( x ) - - r I ~ ( ~ ) g k ( ~ )

by

(ii).

(iv) The integrand AiJkl~kl(iz)~ij(i~ ) 9 ~ -+ IR appearing in the left-hand side of the variational equations over ~ satisfies

(x),

Variational equations in curvilinear coordinates

Sect. 1.3]

31

where (covariant derivatives such as villi have been introduced in (iii))" AiJkl :_ Agij gkl + i~(gik gjl + gil gjk) __ AJikl _ Aklij E C1(~), 1 P - ~Jtl~(") e L 2 ( a ) . ~JlJ(") "= ~("~llJ + vJlr~) - ~1 (Ojvi + Oivj) - r~j,,p We first have, by (iii), 1 1

Since the Christoffel symbols satisfy r ~ - r ~ (c~. (ii)), the functions ek[ll(v) likewise satisfy ekl[t(V ) -- el[ih(v ). Recalling that a ~ ( ~ ) , aJ (=) - g~J (~), we ~e~t h ~

~iJ~ij(iJ)($) - ~ p p ( ~ ) ( $ ) - (ekllt(v)[gk]p[gt]p) ( x ) -

(ekl[t(v)g kI) (x),

and thus

Likewise,

1 (~.~, + ~ . ~ ) ~.(a)(~)~.~(~)(~)- ~.~(~)(~1~.~(~1(~1 : (~ll,(~)~ll.(~)[~],[~']~[~m],[~"]~)(~1 -

(~"~'"~ll,(,,)~mll,,(,,))(~,) 1

since e~ll~(u ) - e~ll~(u ).

(~)

Co,~a~on,.

shows that

Si~c~ d~ - v / ~ ( x i d~ ( T h e .

1.~-1

(~)), part (~)

Three-dimensional linearized elasticity

32

[Ch. 1

on the one hand. At the beginning of this section, it was also shown that the definition of the functions fi and h i implies that

~ ]iv i d~, -- /fi fivi~/r~ dx, f

1

hi~)idr -- ~ hi~i~/Cgd~, 1

on the other, and thus the proof is complete.

m

Naturally, if ~s is identified with I~3 and | -- ida8, each vector gi(x) is equal to ei and thus gi(x) = ~i, g(x) -- 1, giJ(x) - 6 ij, and PiPj(x) - 0 for all m E ~; in addition, the fields (ui) and (fii), (fi) and (]i), (h i) and (hi), and (A ijkl) and (~lijkl) coincide. The variational problem found in Thm. 1.3-1 constitutes the varia t i o n a l , or w e a k , f o r m u l a t i o n of the e q u a t i o n s of t h r e e - d i m e n sional l i n e a r i z e d e l a s t i c i t y in e u r v i l i n e a r c o o r d i n a t e s . The functions A ijkl" -~ -~ I~ introduced in Thm. 1.3-1 are called the e o n t r a v a r i a n t c o m p o n e n t s of the t h r e e - d i m e n s i o n a l elast i c i t y t e n s o r in c u r v i l i n e a r c o o r d i n a t e s ; they thus generalize to arbitrary curvilinear coordinates the components ~ijkt . { ~ } - _+ of the elasticity tensor in Cartesian coordinates (Sect. 1.1). The boundary condition u - (ui) - 0 on r0, or the equivalent relation uig' -- 0 on O(r0), constitutes a (homogeneous) b o u n d a r y c o n d i t i o n of place. o

Remark. The interpretation of the adjective "contravariant" attached to the components of the elasticity tensor is given in Ex. 1.4. m

1.4.

COVARIANT DERIVATIVES AND CHRISTOFFEL SYMBOLS IN A THREE-DIMENSIONAL DOMAIN

We now record as a theorem several important definitions, relations, or properties all originating from the proof of Thm. 1.3-1. Together with those of Sect. 1.2, these constitute our first encounter with differential geometry "in a three-dimensional manifold in IR3 ". Other related notions are treated later, such as the covariant derivatives of

Covariant derivatives and Christoffel symbols

Sect. 1.4]

33

a tensor field (Thin. 1.6-1) and the recovery of a three-dimensional manifold from its metric tensor field (Sect. 1.9).

For further details and complements, see classical texts such as Malliavin [1972], Choquet-Bruhat, Dewitt-Morette & Dillard-Bleick [1977], or Abraham, Marsden & Ratiu [1983]. The books by Green & Zerna [1968], Marsden & Hughes [1983], and Simmonds [1994] provide treatments of differential geometry and tensor analysis that are essentially motivated by, and thus well adapted to, three-dimensional elasticity. T h e o r e m 1.4-1. Let the assumptions on the mapping 19 and the definitions of the vector fields gi and gJ be as in Thm. 1.3-1, and let there be given a vector field rig 2 on f~ with smooth enough covariant components vi 9f~ --~ ~. (a) The components of the vectors gi(x) and gJ(x) are given by

=

In other words, the components of g i ( z ) are those of the i-th column of the matriz V O ( z ) while those of gJ(z) are those of the j-th row of the matriz V 0 ( ~ ) . (b) The f i r s t - o r d e r covariant derivatives Villi " f~ --~ I~ of the vector field rig', which are defined by ^

^

p ._ gp Villi : : Ojvi - r ipj v p, where Fij "Oigj,

can be also defined by the relations

(c) The Christoffel symbols satisfy the relations

::

g

.Oig

OigP - - r pij gJ and 0j gq - rjqgi" i

-

.

Three-dimensional linearized elasticity

34

(d) Let r

[Ch. 1

i be the vector field defined on {fi}- - - |

by

~i(~)~ i : - vi(x)gi(x) for all ~ - O(x), x e ~, and let [gk(x)]i denotes the i-th component of gk(x) over the basis {el, e2, &z}. Then, for all x E f~,

~j~)i(~,) - (Vklll[gk]i[gl]j) (X), X -- O(X). II

Proof. It remains to verify that the covariant derivatives Villi, defined in part (iii) of the proof of Thm. 1.3-1 by p

Villi -- Ojvi -- rijv p, may be equivalently defined by the relations

Oj(vig i) --

Villjg i,

which unambiguously define the functions the vectors gi are linearly independent at tion. To this end, simply note that, by symbols satisfy Oigp - - r P .3g j (eL part 1.3-1); hence

oj(,ig i) - ( o j , i ) g i +

Villi -- ( O j ( v k g k ) } "gi since all points of ~ by assumpdefinition, the Christoffel (ii) of the proof of Thin.

~ia~g ~ - (aj V i)g i - ~ i r j ki g k -~illjg'."

i note that To establish the other relations Ojgq - r jqgi, 9

0 - Oi(g p . g q ) - -F~ig~.gq + g P . Oig q

_

-r~j + gp .Ojg~; p

hence

Ojgq -- (Ojgq.gP)gp -- rpqjgp" II If the affine space C3 is identified with IR3 and 19 - id, the relation COj(vigi)(x) -- (Villjgi)(x) found in Thm. 1.4-1 (b) reduces to

~j(~)i(x)e i)

-

-

(Oj~)i(x))e, i. In this sense, a covariant derivative of the

Sect. 1.5]

Linearized change of metric tensor in curvilinear coordinates

35

first order constitutes a generali~,ation of a partial derivative of the first order in Cartesian coordinates. Remarks. (1) The relation between the functions 0jvi and Vklll (Tam. 1.4-1 (d)) can be inverted; cf. Ex. 1.5. (2) The formula

established in part (iv) of the proof of Thm. 1.3-1, is the expression of the divergence of a vector field in curvilinear coordinates. Formulas likewise expressing the gradient, curl, and Laplacian operators in curvilinear coordinates are given in Ex. 1.6. m 1.5.

LINEARIZED CHANGE OF METRIC CURVILINEAR COORDINATES

TENSOR

IN

Let there be given an arbitrary d i s p l a c e m e n t field of the set O(fl), i.e., an arbitrary vector field rig z defined by means of its cov a r i a n t c o m p o n e n t s vi" ~ ~ R; this means that vi(x)gi(x) is the displacement of the point ~ = O (z). We then show that the matrix 1

p

vi + Oiv~) - ri~vp),

introduced in Thm. 1.3-1, generalizes to arbitrary curvilinear coordinates the linearized strain tensor

in Cartesian coordinates (Sect. 1.1). More specifically, we show that the matriz (eillj(V)) likewise measures (half of) the linearized difference between the "new" metric in the deformed configuration ( 0 + vigi)(-~) and the "old" metric in the reference configuration O(~), but now expressed by means of their covariant components in terms of the curvilinear coordinates xi. We also record for future reference the relation between the functions ~j(~) and ekllt(v) that was established in part (iv) of the proof of Thm. 1.3-1 (this relation can be inverted; cf. Ex. 1.5).

Three-dimensional linearized elasticity

36

[Ch. 1

T h e o r e m 1.5-1. Let f~ be a domain in I~3, let 19 :-0 --> E 3 be a smooth enough injective mapping such that the three vectors gi = Oi| are linearly independent at all points of-0, and let the vectors gi be defined by g i . g j = ~ . Given an arbitrary displacement field

V" :--

V

ig i

w

of the set | with smooth enough covariant components vi" f~ ~ I~, let the e o v a r i a n t c o m p o n e n t s of the l i n e a r i z e d s t r a i n , or line a r i z e d c h a n g e of m e t r i c , t e n s o r associated with this vector field be defined by 1 eillj(V ) := ~[ffij(V) -- ffij] fin

where 9ij and 9ij(v) denote the covariant components of the metric tensors respectively attached to the sets 19(-0) and (19 + vigi)(-~), and [...]tin denotes the linear part with respect to v := (vi) in the ezpression [...]. Then

eillj(v)

-

~

" gi

"gj

(v)

1 = ~(vill j + Villi) = 2

- Pv.._--_~.,,3

P p " - O ~ I ~ and Fij p 9-where the functions Villi - O j v i - Fijv f~ ~ R are respectively the first-order covariant derivatives of the vector field rig i and the Christoffel symbols of the surface S (Thin. 1.4-1). The functions eillJ(V ) are also called the l i n e a r i z e d s t r a i n s in e u r v i l i n e a r coordinates. The linearized strains in Cartesian and curvilinear coordinates are related by:

.=

:

-

Sect. 1.6]

Boundary value problem in curviIinear coordinates

37

Proof. The covariant components gij (v) are defined in ~ by (Sect. 1.2)

g,j(~) : o~(| + ~). oj(|

+ ~).

Note that both the reference configuration O(~) and the deformed configuration (| + ~)(12) are equipped with the same curvilinear coordinates xi. The relations o~(| + ~) : g~ + O~ then show that

= g~j + oj~ 9g~ + 0 ~ 9gj + o ~ . oj~, hence that 1

- ~l ( 0 j ~ "g, + o ~

. g j .)

The other expressions of the functions eillj(V) follow from the relations 0j~ - vklljg k and vkllj - Ojvk - r j kpvp (Thm. 1.4-1). m

1.6.

THE BOUNDARY VALUE PROBLEM OF THREE-DIMENSIONAL LINEARIZED ELASTICITY IN CURVILINEAR COORDINATES

While deriving the boundary value problem that is (at least formally) equivalent to the variational equations of three-dimensional linearized elasticity in Cartesian coordinates simply amounts to applying the fundamental Green formula, doing so in curvilinear coordinates is more subtle. As we next show, it relies in particular on the notion of covariant differentiation of a tensor field. We recall that ni(x)e i denotes the unit outer normal vector at x E r and that f i E L2(~) and h i C L2(r~) by assumption.

Three-dimensional linearized elasticity

38

[Ch. 1

T h e o r e m 1.6-1. Let the notations and assumptions be as in Thm. 1.3-1. If the solution u = (ui) to the variational problem: E V(~):=

{V = (Vi) E Hl(fl); v = 0 on r 0 } ,

f A'Jk~ekll,(u)e~ll~(v)v/~dz=fi'vi~dz+frh%~dr for all v = (vi)E V(f~), 1

is smooth enough, it also satisfies the following b o u n d a r y v a l u e p r o b l e m of t h r e e - d i m e n s i o n a l l i n e a r i z e d e l a s t i c i t y in e u r v i linear coordinates: -~ilj-f

~ in

f~,

on

r0,

ui -- 0

where the functions oriJ :--- AiJktekllt(u )

are the c o n t r a v a r i a n t c o m p o n e n t s sor field, and the functions

of the l i n e a r i z e d s t r e s s t e n -

are f i r s t - o r d e r e o v a r i a n t d e r i v a t i v e s of this tensor field (naturally, r jjq - ~j:~3 rjq~ when k - j according to the summation convention)

Proof. (i) We first establish the relations (needed in part (ii)): q

To this end, we recall that x/~ - I det V{91, that the column vectors of the matrix V | are 01, 09., g3 (in this order), and that the vectors gi are linearly independent at all points in f~. Assume for instance that det V | > 0, so that V~ : det V O : det(gl, g2, g3) in f~.

Boundary value problem in curvilineav coordinates

Sect. 1.6]

39

Then

OjX/~- det(0jgl, g2, g3)-1-det(gl, Ojg2, g 3 ) + det(gl, g2, Ojg3) - r~j aet(g,, g2, g~) + r~j aet(gl, g~, g~) + r[j aet(g~, g~., g~) P (Thm. 1.4-1 (c)); hence since 0jgq - rqjgp

0 j @ - (r b + r~j + r~j)det(ffl,

if2, if3) -

r~j ~4~.

The proof is similar if v / ~ - - d e t ~ ' O in f~. (ii) Assume that the functions a ij are in Hl(f~) (as is the case if u E H2(f~) and the assumptions on the mapping O are those of Thm. 1.3-1), so that we can apply the following Green formula in Sobolev spaces (see, e.g., Vol. I, Thm. 6.1-9)"

ff(Ojv)wdx - - ff vOjwdx+ frVWnjdF f~ all v, w E Hl(f~)" Taking also into account the symmetries crij - orJi (which themselves follow from the symmetries A ijkl - AJikl; cf. Thm. 1.3-1) and q (part (i)), weobtain: the relations 0j x/~ - V~ rqj

fn AiJkleklll(u)eillj(v)v/g dx - / ~ aiJeillj(v)v~ dx a =

.. 1

p _

rijvpdx

-- - ~ Oj (~criJ)vi dx + fr v~aiJnjvi dr - ~ ~apJripjvi dx

----ff~ %//g(Ojo'iJ-~- FipjaPJ+ r~qaiq)vidx+ fr %//-goriJnjVidr

for all v - (vi) C Hl(f~). Hence the variational equations imply that

fnr

(~J [Ij +/*) v, dx - fr 4~ (~iJnj - h*) v~ dr 1

Three-dimensional linearized elasticity

40

[Ch. 1

for all (vi) E V(f~). Letting the functions Vi vary in ~ ( f t ) shows t h a t crijiij + f i _ 0 in f~ and letting the functions (vi) vary in V(ft) in the remaining equations shows that aiJnj - h i - 0 on F l, m Naturally, the same b o u n d a r y value problem in curvilinear coordinates can be directly obtained from its Cartesian counterpart: __~j~iJ

=

~2i --

&ij hj

-

]i

in ~,

0

on on

hi

I'o, FI,

where &ij _ f~ijkl~kl(~t ) (Sect. 1.1); but again this requires some care; cf. Ex. 1.7. The variational equations

aiJeillJ(v)~/~ dx -- ffl fivi~/rg dx -f- f r h i v i v ~ d r 1

for all v = (vi) E V ( ~ ) constitute the linearized principle of virtual w o r k in c u r v i l i n e a r c o o r d i n a t e s . The equations

- ~ i ~ l l j - f ~ in cri] nj -- h i

on

f~, F1,

constitute the linearized equations of equilibrium in c u r v i l i n e a r coordinates. 1.7.

A LEMMA

O F J . L. L I O N S ;

THREE-DIMENSIONAL KORN'S INEQUALITIES AND INFINITESIMAL RIGID DISPLACEMENT LEMMA

IN CURVILINEAR

COORDINATES

We first review some essential definitions and notations, together with a fundamental lemma of J.L. Lions (Thm. 1.7-1); we borrow here the beginning of Sect. 1.1 from Vol. II. A domain ft in IRn is an open, bounded, connected subset of IRn with a Lipschitz-continuous boundary F - Of~, the set ft being locally

Korn's inequalities in curvilinear coordinates

Sect. 1.7]

41

on one side of F. As F is Lipschitz-continuous, a measure elf can be defined along F and a u n i t o u t e r n o r m a l v e c t o r v = (vi) ni--1 ("unit" means that its Euclidean norm is one) exists dF-almost everywhere along F (see, e.g., Vol. I, Sect. 1.6). For the same reason, the classical spaces Cm(f~) or Cm' a (f~), 0 < c~ < 1, can be unambiguously defined for any integer m > 0; see, e.g., Ne~as [1967, Chap. 2], Adams [1975, Chap. 1], Stein [1970]. Let f~ be a domain in I~n. For each integer m > 1, Hm(f~) and H~ n(f~) denote the usual S o b o l e v s p a c e s ; in particular,

HI(~) "- {~ E L2(~); Oi~ E L2(~), 1 < i )] < v, qo > l - l fnvqodxl 1-!-

< v, oil, > 1 -

- f. vOi dx I _ 1, eillj(vk)qo dx - _ ff~ {-~l (vki Oj q~ + vjkOiqo) + rijvpqo shows that eillj - eillj(v ). (ii) The spaces W(f~) and H 1(f~) coincide. Clearly, Hl(f~) C W(f~). v - ( v i ) e W(f~). Then

%(v)

To establish the other inclusion, let

v := ~1 (Ojvi + Oivj) - (el IIJ(v) + rijvv}

since eillj(v ) C L2(f~), r ip C C~

~ L2(f~),

and vp C L2(f~). We thus have OkVi E H - I ( ~ ) ,

o j ( o k ~ ) - {oj~/k(~) + oh~/j(~) - o ~ j k ( ~ ) } e H - ~ ( ~ ) ,

since w E L2(f~) implies Okw e H-l(f~). Hence Okvi C L2(f~) by the lemma of J.L. Lions (Thm. 1.7-1) and thus v e Hl(fl). (iii) Korn's inequality without boundary conditions. The identity mapping t from the space H I ( ~ ) equipped with I1" II1,• into the space W ( G ) equipped with I1" I1~ is injective, continuous (there clearly exists a constant c such that [[v[[~ < cllvlll, n for all v C Hi(G)), and surjective by (ii). Since both spaces are complete (cf. (i)), the closed graph theorem (see, e.g., Brezis [1983, p. 19] for

46

Three-dimensional linearized elasticity

[Ch. 1

a proof) then shows that the inverse mapping 5-1 is also continuous; this continuity is exactly what is expressed by Korn's inequality without boundary conditions. II Our next objective is to "get rid" of the norms ]vilo, n in the righthand side of the Korn inequality established in Thm. 1.7-2 when the fields v - (vi) E t t l ( f l ) are subjected to the boundary condition v = 0 on r0 C r and area r0 > o. As a preliminary, we establish the weaker property that the semi-norm v--+

i,j

becomes a n o r m for such fields, by generalizing to curvilinear coordinates the well-known infinitesimal rigid displacement l e m m a in Cartesian coordinates (see, e.g., part (ii) of the proof of Thm. 6.3-4 in Vol. I); "infinitesimal" reminds that if eillj(v) - 0 in fl, i.e., if only the linearized part of the change of metric tensor vanishes, the corresponding displacement field rig i is likewise only the linearized part of a genuine rigid displacement (for more details in Cartesian coordinates, see Vol. I, Ex. 6.2). Part (a) in the next theorem is an infinitesimal rigid displacement l e m m a "without boundary conditions"~ while part (b) is an infinitesimal rigid displacement lemma "with boundary conditions". 1.7-3 ( i n f i n i t e s i m a l rigid d i s p l a c e m e n t l e m m a in e u r v i l i n e a r c o o r d i n a t e s ) . Let the assumptions be as in Thm. 1.7-2. (a) Let v = (vi) e I'II(f~) be such that Theorem

eillJ(V ) - 0 in ft. Then the vector field r i g i iS an i n f i n i t e s i m a l r i g i d d i s p l a c e m e n t , in the sense that there ezist two vectors ~, tl C N 3 such that

vi(x)gi(x) - ~-4-d A O(x) for all x E ~, (b) Let ro be a dF-measurable subset of r = Of~ that satisfies area r o > O.

Sect. 1.7]

Korn's inequalities in curvilinear coordinates

47

Then v--

(vi) E

HI(f~), v =0 onr0, } ~ v = 0 inf,. eillj(V )

--0 in f~

Pro@ In part (iv) of the proof of Thm. 1.3-1, we established the relation ~ii(@)(&) - (ekll,(V)[gk]i[gt]j)(x)

for all ~ - |

x E ~2,

where gij(i~) : 89162 + Oivj) and the vector fields ~ -- (~3i) E I-II(h) and v - (vi) E H I ( ~ ) are related by

~i(&)~ i - vi(x)gi(x) for all & - |

x e f~.

Hence and the identity (the same as in the proof of Thm. 1.7-2) c~i(vSk~i) - 0i~ik(v) + 0keii(v) - c~ieik(v) in T~'(~) further shows that eij(~)) -- 0 in (2 ::ff Oj(Ok~)i) -- 0 in ~)'((2).

By a classical result from distribution theory (Schwartz [1966, p. 60]), each function Oi is therefore a polynomial of degree < 1 (recall that the set ~ is connected). In other words, there exist constants ci and dii such that

~i(~.) - c.i + dij~j for all ~ - (~i) C ~. But eij(v) - 0 also implies that dii vectors ~, d E IR3 such that

-dii; hence there exist two

i~i(~.)~ i - ~. + (/A O ~ for aU ~

E ~,

hence such that

vi(x)gi(x) - & + (~ A O ( x ) for all x C C~.

Three-dimensional linearized elasticity

48

[Ch. 1

Since the set where such a vector field Vi ~i vanishes is always of zero area unless ~ -- d = 0 (as is easily proved; see, e.g., Vol. I, T h m . 6.3-4), it follows that ~ - 0 when area ro > O. I Remarks. (1) Since the fields gi are of class C 1 on ~ by assumption, the components vi of a field v = (vi) E Ht(f~) satisfying eillj(v) = 0 in f~ are thus automatically in C1(~) since vi - (vjg j) "gi.

(2) Remarkably, the field rig i - fi + d A O inherits in this case even more regularity, as it is of class C2 on ~ (a similar p h e n o m e n o n will be encountered in Thm. 2.6-3)! (3) The assertion in part (a) illustrates a key idea from differentim geometry' An "intrinsic" property (the vector field rig z is an infinitesimal rigid displacement) is derived from relations (the assumptions eilij(v) - 0 in f~) written in a particular system of curvilinear coordinates. 1 We are now in a position to prove a K o r n inequality "with boundary conditions", which plays a fundamental r61e in three-dimensional linearized elasticity in curvilinear coordinates (Thm. 1.8-2). T h e o r e m 1.7-4 ( K o r n ' s i n e q u a l i t y in c u r v i l i n e a r c o o r d i n a t e s ) . Let f~ be a domain in I~3 and let 0 be a C2-di~eomorphism of-~ onto { ~ } - - O ( ~ ) , so that the three vectors gi - OiO are linearly independent at all points of f~, let ro be a dP-measurable subset of F = Of~ that satisfies

area I'0 > 0,

and let the space V(f~) be defined by

V(fl)

:= {v -

(v,) c

H~(fl);

v - o

on

r0}.

Then there exists a constant C = C(f~, t o , O) such that

'}

{

IlVlll,a ~ C ~ ]eilij(v)10,a i,j

~/z for all v C V(f~).

Sect. 1.7]

Korn's inequalities in curvilinear coordinates

49

Proof. Given v --(vi) e HI(f~), let 2

I~1.'= ~le, llj(~)lo,.

}1/2

i, j

If the announced inequality is false, there exists a sequence (v k ) koo= 1 of elements v h E V ( ~ ) such that ""llvklll,~ = 1 for all k and

Since the sequence

(vk)~~

lira [vki~ = 0.

k--+oo

is bounded in Hi(12), a subsequence

(Vl)~~ 1 c o n v e r g e s in L2(~/) by the Rellich-Kondragov theorem (see,

e.g., Vol. I, Thm. 6.1-5); furthermore, since liml~oo Ivt[n - 0, each sequence (eilj(vl))~l also converges in L2(f~) (to 0, but this information is not used at this stage). The subsequence (v l ) ~ l is thus a Cauchy sequence with respect to the norm }1/2

-(vi) -+ ~ [~il02. + ~ leijjj(~)l~o,. i

i,j

hence with respect to the norm II. IIx, n by Korn's inequality without boundary conditions (Thm. 1.7-2). The space V(f~) being complete as a closed subspace of Hl(f~), there exists v E V(f~) such that v I --+ v in Hi(12), and the limit v satisfies leillj(V)]0,~ = limt~oo le~ll~(Vt)10,~ - 0; hence v - 0 by Thin. 1.7-3. But this contradicts the relations IIv~llx,~ - 1 for all I > 1, and the proof is complete, m Identifying E 3 with I~3 and letting O - idR8 shows that Thms. 1.7-2, 1.7-3, and 1.7-4 contain as special cases the Korn inequalities and the infinitesimal rigid displacement lemma in Cartesian coordinates (see, e.g., Duvaut & Lions [1972, p. 110], Vol. I, Sect. 6.3, or Vol. II, Sect. 1.1).

50

[Ch. 1

Three-dimensional linearized elasticity

1.8.

EXISTENCE AND UNIQUENESS CURVILINEAR COORDINATES

THEOREM

IN

As a preliminary to showing that the bilinear form found in Thm. 1.3-1 is V(f~)-elliptic, we first need to establish the uniform positive definiteness of the three-dimensional elasticity tensor ("uniform" means with respect to points in f~ and to symmetric matrices of order three). Incidentally, the proof of this property has a flavor typical of differential geometry: Although the proof is seemingly innocuous, it may not be that innocuous to find (the reader should verify this assertion)! T h e o r e m 1.8-1. Let the assumptions on the mapping (9 be as in Thm. 1.3-1, let the contravariant components A ijkl 9-~ -+ I~ of the

elasticity tensor be defined by A i J k t _ Agijgkt + #(gik gfl + gil gjk),

and assume that )~ >_ 0 a n d # > O.

Then there exists a constant Ce = Ce(f~, (9, #) > 0 such that [tijl z _C~Ic-2v~o[lv]]~,n for all v C V(f~).

54

Three-dimensional linearized elasticity

[Ch. 1

Hence the bilinear form is V ( ~ ) - elliptic. The bilinear form being also symmetric since A ijkt = A ktij, all the assumptions of the Laz-Milgram lemma in its "symmetric" version (see, e.g., Vol. I, Thm. 6.3-2) are satisfied: The variational equations have one and only one solution, which may be equivalently characterized as the solution of the minimization problem stated in the theorem, m An immediate corollary with a more "intrinsic" flavor to the above result is the existence and uniqueness of a displacement field uig i, whose covariant components ui E H i ( n ) are thus obtained by finding the solution u = (ui) to the variational problem of Thm. 1.8-2. Since the vector fields 9i of the contravariant bases belong to the space C1(~) by assumption, the displacement field uig i also has its Cartesian components in H 1(fl). Naturally, the existence and uniqueness result of Thm. 1.8-2 implies the same result in Cartesian coordinates (to see this, identify E 3 with I~a and let O - idR3). The converse implication also holds; cf. Ex. 1.10.

Remarks. (1) When I'0 = F and the boundary r is smooth enough, regularity results can be obtained, showing that the weak solution obtained in Thm. 1.8-2 is also a "classical solution", i.e., a solution of the corresponding boundary value problem (Thin. 1.6-1); cf. Ex. 1.11. (2) The assumptions ]i E L2(~) and ]~i e L2(?l) made for definiteness in Sect. 1.1 can be slightly weakened as in Thm. 1.8-2, to ]i e L6/5(~) and hi e L4/3(rl). m 1.9 b.

C O M P L E M E N T : R E C O V E R Y OF A THREE-DIMENSIONAL MANIFOLD METRIC TENSOR FIELD

FROM ITS

Let ~ be an open subset in IR3 and let O : ~ -+ E 3 be a thrice continuously differentiable mapping such that the three vectors g i = 0 i 0 are linearly independent everywhere in ~. As before, let gij - 9 i ' g j , let the three vectors gJ be defined by the relations

gJ "gi - ~ , let gij _ 9 i . 9j and finally, let the Christoffel symbols be defined by Fi~ - 9P. ~jgi. It is easily found that the Christoffel

Recovery of a three-dimensional manifold

Sect. 1.9b]

55

symbols satisfy the following compatibility conditions (Ex. 1.12):

o~r ~ - o~ r~, + r,"~r ~ , - r ~ r~k - o i~ ~. These conditions are in effect relations between partial derivatives of the first, second, and third order of the mapping | They are also relations between the functions gij and their derivatives, since the Christoffel symbols r i~ themselves may be directly defined in terms of the functions gij as follows (Ex. 1.12):

r,~ - F ~ r , j ~ , where

rijq

:=

1

-~(Ojgiq + Oigjq -

Oqgij).

The functions rijq a r e called the Christoffel symbols of the first kind and the functions r pi are called in this context the Christoffel symbols of the second kind. The above compatibility conditions may also be expressed in terms of the Christoffel symbols of the first kind as (Ex. 1.12): O l r i k j -- o k r i l j -4- gmn(rit~rjkm - r i k , r j t m ) = 0 in f~.

Remarkably, these necessary conditions (in either one of their equivalent forms) are also sufficient for the existence of a mapping {9 : f~ C R 3 --> E 3 whose metric tensor field is given on f~: T h e o r e m 1.9-1. Let f~ be a simply connected open subset of ~3, and let there be given a twice continuously differentiable, symmetric, and positive definite matrix field (gij) on f~ that satisfies

otrikj - okrilj + g~"(ri~.rjk~

- rik.rj~m)

- o i n f~, w h e r e

1

Then there exists a mapping | C C3(f~; 1~3) such that Oi| . Oj | = gij in ft. Furthermore, this mapping is unique "up to rigid deformations in R 3 ": This means that any other solution is necessarily of the form

56

Three-dimensional linearized elasticity

[Ch. 1

x E f~ --+ e + Q| where e is a vector in I~3 and Q is an orthogonal matrix of order three. This result is a consequence of the compatibility relations satisfied by the Christoffel symbols, of the simple connexity of f~, and of a deep existence result of Thomas [1934]; see Blume [1989]. EXERCISES

1.1. Compute the vectors of the covariant and contravariant bases, the volume, area, and length elements, the Christoffel symbols~ and the covariant and contravariant components of the metric tensors (Sect. 1.2) corresponding to cylindrical and spherical coordinates (Fig. 1.2-3). 1.2. This exercise explains in what sense the components of a vector may be "covariant" or "contravariant". Let f~ and ~ be two domains in I~a and let @ 9~ ~ E a and @ 9 { ~ ) - ~ E s be two Cl-diffeomorphisms such that | - @(~) and such that the vectors g i ( x ) " - 0i@(x) and ~)i(&) - 0i@(~) of the covariant bases at the same point @(x) - ~)(~) - & e { ~ } are linearly independent. Let gi(x) and ~i(~) be the vectors of the corresponding contravariant bases at the same point &. (1) Show that gi(x)-

where X -

0X i g~ ~-~X/(X)gj(X) and ( x ) -

(X i) :=

~-x

0;~~ ~(~)~i(~)

o @ 9~ -~ { ~ } - (hence ~ - X(X)) and

( ~ ) . - x - ~ . {fi}- -+ ~.

(2) Let vi(x) and vi(x) be the covariant components and let vi(x) and ~i(~) be the contravariant components of the same vector at ~, i.e., ~(:)g~(:)

- ~i(~W(~)

- ,~(:)g~(~)

-

r

Show that

~(~)-

~OXi (x)6i(~ ) and v i ( ~ ) -

0 ~ ~ (~)~i(~)

In other words, the components vi(x) "vary like" the vectors 9 i ( x ) of the covariant basis under a change of curvilinear coordinates, while

Ezercises

57

the components vi(x) of the same vector "vary like" the vectors gi(x) of the contravariant basis: This is why they are respectively called "covariant" and "contravariant". 1.3. This exercise shows why the "covariant" and "contravariant" components of the metric tensor are so named. The notations and assumptions are those of Ex. 1.2. Let gij (x) and gij (&) be the covariant components and let gij (x) and ~z3(&) be the contravariant components of the metric tensor (Sect. 1.2) at the same point @(x) - @)($) - ~ e { ~ } - . Show that .

.

0x k

0x ~

g i j ( x ) - -~xi(x) ~

9 0~ ~ 0~J )~k~ (x).qkl(~) and g,3 ( x ) - ~ ( x ) - ~ l (x (x)"

These formulas explain why the components gij(x) and gij (x) are respectively called "covariant" and "contravariant": Each index in gij (x) "varies like" that of the corresponding vector of the covariant basis under a change of curvilinear coordinates (see Ex. 1.2 (1)), while each exponent in gZ3(x) "varies like" that of the corresponding vector of the contravariant basis (see ibid.).

Remark. What is exactly the "second-order tensor" hidden behind its covariant components gij(x) or its contravariant exponents gij (x) is beautifully explained in the gentle introduction to tensors given by Antman [1995, Chap. 11, Sects. 1 to 3]; it is also shown in ibid. that the same "tensor" also has "mixed" components g~(x), which turn out to be simply the Kronecker symbols (f~! Exhaustive treatments of tensor analysis, particularly as regards its relevance to elasticity, may be found in Boothby [1975], Marsden & Hughes [1983, Chap. 1], or Simmonds [1994]. 1.4. The assumptions are those of Ex. 1.2. 1 (1) Let ~iJk(x) if {i, j, k} is an even permutation of {1, 2, 3}, let eiJk(x) -

1

V/g(x ) if {i, j, k) is an odd permutation of

{1, 2, 3), and let eiJh(x) - 0 otherwise. Show that each exponent in the functions eiJk(x) "varies like" that of the corresponding vector of the contravariant basis under a change of curvilinear coordinates. (2) Show that each exponent in the "contravariant" components AiJkt(x) of the three-dimensional elasticity tensor in curvilinear co-

58

Three-dimensional

[Ch. 1

linearized elasticity

ordinates introduced in Sect. 1.3 again "varies like" that of the corresponding vector of the contravariant basis under a change of curvilinear coordinates.

Remark. See again Antman [1995, Chap. 11, Sects. 1 to 3] to decipher the "third-order tensor" and "fourth-order tensor" hidden respectively behind their contravariant components s ijk (x) and AiJkt(x). 1.5. In part (iii) of the proof of Thm. 1.3-1, it is shown that

Show that, conversely, each covariant derivative vilfj(x) can be expressed as a linear combination of the partial derivatives 0tvk(x). 1.6. This exercise provides the expression of the gradient, Laplaclan, and curl operators in curvilinear coordinates (that of the divergence operator is given at the end of Sect. 1.4). The notations and assumptions are those of Thm. 1.3-1. (1) Given a function 9" 12 -4 1~, let gra~"d~ be the vector field with 029 components Oil), let ~ "-0-~, and let the function v" f~ -4 R

-,~

b e defined by v(x) - 6($) for all ~ - @(x) C ~. Show that

(gr."--a ~)(~) -

A~(~) -

((o,~)g')

(.),

(1~o~(~g',o~) .. ) (~).

(2) Given a vector field ~ - (~i) 9 fi -~ N 3, let e u r l ~ be the vector field with components gOkOj~i, where gob _ +1 if {i, j, k} is an even permutation of {1, 2, 3}, gOk = - 1 if {i, j, k} is an odd permutation of {1, 2, 3}, and g i j k _ 0 otherwise. Show that

cur~l,~(~) - (~Jk~jll~gk)(~), 1 where eiJk(x):= ~ g i j k .

Jg(.)

1.7. Show that the boundary value problem of three-dimensional linearized elasticity in curvilinear coordinates (Thm. 1.6-1), viz., -aO[[j

_

fi

in 12,

ui - 0 on r0,

"" a2Jnj

--

h i on r l ,

Ezercises

59

where a ij - AiJhtekllt(U), can be directly derived from its Cartesian counterpart (Sect. 1.1), viz.,

_3j&ij _ ]i in h, ui - 0 on r0, &iJhj - ~i on F1, where &ij _ ~ijkt~kt(i, ) ("directly" means without recourse to the variational equations as in Thm. 1.6-1). 1.8. The notations and assumptions are those of Thm. 1.8-1. Letting t i ( x ) : = tijg j(x) and [ti(x)]J := ti(x). ~J, show that gik( )gJl( )tk t j

I[ti( )]Jgi( )12

--

J Then infer from this equality another proof of this theorem. 1.9. (1) Show that the three-dimensional elasticity tensor in Cartesian coordinates, defined in Sect. 1.1 by its components

remains positive definite "even if )~ is slightly negative", in the following sense: There exists a constant (7 > 0 such that

~ijkt tkttij ^ ^ >__0 ~

Itijl 2 for all symmetric matrices (tij)

i,j

if and only if/z 3> 0 and 2A + 3/, > 0. (2) Show that a similar property holds for the elasticity tensor defined in curvilinear coordinates by its contravariant components

Aijkl _ Agij gkt + lz(gik gjt + gil gjk). 1.10. Combining the relation (Thm. 1.3-1)

d~ - fn Aijktekllt( u )eillj ( v ) v/g dx with the three-dimensional Korn's inequality in Cartesian coordinates (see, e.g., Vol. I, Sect. 6.3 or Vol. II, Sect. 1.1), show directly that the bilinear form

.) e v(n) • v(n) -+ fn A ijktekllt(u)eillj(v)~/~ dx

Three-dimensional linearized elasticity

60

[Ch. 1

is V(f~)-elliptic, thus providing another proof to Thm. 1.8-2.

Hint: Use a classical result about composite mappings in Sobolev spaces (see, e.g., Ne~as [1967, Chap. 2, Lemma 3.2] or Adams [1975, Thm. 3.35]). 1.11. (1) Show that, if the boundary r and the mapping 19 are sufficiently smooth, if r0 - r , and if fi E LP(f~), p > 6 the weak solution u E V(f~) - H01(f~) found in Thm. 1.8-2 is in the space (2) Show that u satisfies the equations (Thm. 1.6-1)

--AiJklekllt(u)llj

_ fi

in LP(f~).

Hint: Use the regularity of the weak solution of the corresponding boundary value problem of three-dimensional linearized elasticity in Cartesian coordinates (Vol. I, Thin. 6.3-6). 1.12. (1) Show that the Christoffel symbols of the second kind satisfy the relations m j

m j

(2) In the text, the Christoffel symbols of the second kind are defined as r,5 : 0jg, (Thm. 1.4-1), i.e., by means of the vectors of the covariant and contravariant bases. It is remarkable that they can also be defined in terms of the covariant and contravariant components of the metric tensor. More precisely, show that

-

where

rij

1 .=

(Ojgiq q- Oigjq - -

Oqgij).

(3) Show that the relations satisfied by the Christoffel symbols of the second kind (cf. (1)) may be equivalently expressed in terms of the Christoffel symbols of the first kind as

olrikj - okrilj + gm~ (ritnrjkm --

riknrj )

- o in ~.

CHAPTER 2 INEQUALITIES

OF KORN'S

TYPE

ON SURFACES

INTRODUCTION We shall see in the next chapters that the theory of linearly elastic shells leads to two-dimensional equations that are "posed on the middle surface S of the shell", i.e.~ that are expressed in terms of curvilinear coordinates of the surface S. The purpose of this chapter is to study such equations per themselves. To this end, we first provide all the necessary preliminaries from the di~erential geometry of surfaces in It~3 (Sects. 2.1 to 2.3). We then provide complete proofs of the existence and uniqueness of the solutions to three fundamental classes of linear shell equations, the elliptic membrane, flexural, and Koiter equations (Sects. 2.6 and

2.7). As in Chap. 1, the treatment is entirely sel]-contained, in that no a priori knowledge of differential geometry is assumed. More specifically, recall that a "three-dimensional manifold" 0(12) in IR3, where 12 is a three-dimensional domain in I~3 and O 9~ -+ I~3 is an ad hoc injective mapping, is unambiguously defined (up to rigid deformations) by a single tensor field~ the metric tensor field~ whose covariant components gij - gji " 12 ~ R are given by gij - 0 i O . 0 j O (cf. Sects. 1.2 and 1.9). Consider instead a surface S - 8(~) in I~3 where w is a two-dimensional domain in I~2 and 8 9 ~ -+ I~~ is a s m o o t h injective mapping with other ad hoc properties. T h e n by contrast, such a "two-dimensional manifold" requires two tensor fields for its definition (again up to rigid deformations)~ the metric tensor field and the curvature tensor field, whose covariant components aafj = af~a : w -+ I~ and bar3 = bf3a : w -+ IR are respectively given by (Greek indices or exponents take their values in {1, 2}):

aa~ = aa " aft and bail = a3 9Oaa~, where a a - 0 a e and a3 -

a l Aa2 la 1 A a21" These two tensors, which are

also called the first and second ]undamental forms of the surface, are studied in Sects. 2.1 and 2.2; see also Sect. 2.8.

62

[Ch. 2

Inequalities of Korn's type on surfaces

In Sects. 2.4 and 2.5, we introduce two other fundamental tensors, which play a key rble in the two-dimensional theory of linearly elastic shells, the linearized change of metric tensor and the linearized change of curvature tensor, each one being associated with a displacement vector field ~Tiai of the surface S = O(~). where the vectors a i are defined by the relations a i . a j = ~ . The covariant components of these tensors are given by 1 p.~(.)

-

oo~0~ - r ~o~o~0~ - b~b~,~ + b;(O~,~ - r ~ , ~ )

+b~(0~.~ - r ~ . ~ )

+ (0~b~ + r ~ b 3 - r ~

~

where F~f3 - aa.Oaaf~ are the Christoffel symbols of S (Sect. 2.3) and /fin are the mixed components of the curvature tensor of S (Sect. 2.2). The functions 7af3(rl) and paf3(r/) may be also written in more condensed manners, either by means of covariant derivatives or through the introduction of the vector field yia* (Thms. 2.4-1 and 2.5-1). Note that

7o~(~) c L2(~)

i~ ~ -

( ~ ) c H~(~) • H~(~) • L~(~),

An inequality of Korn's type "on a general surface" is then established (Thin. 2.6-4): Given arty subset 70 of 7 = Ow satisfying 0 < length 70 < length 7, define the space

vx(~)

= {~ - (0~) e H ~ ( ~ ) • H ~ ( ~ ) • g 2 ( ~ ) ; ~ = 0 ~

= 0 o . ~0}.

Then this inequality asserts the existence of a constant c such that 2

x,,,, + fir/3 ]12,,,, O~

a,f3

2

}1/2

a,f~

fo~ an ~ = (~) e v x ( ~ ) . The existence and uniqueness of a solution to the two-dimensional Koiter equations for a linearly elastic shell and to the two-dimensional equations of a linearly elastic flexural shell follow from this inequality. We also show how this inequality of Korn's type has been recently extended to surfaces "with little regularity" (Thm. 2.6-6). If 70 = 7 and the surface S is elliptic, i.e., both principal radii of curvature are everywhere of the same sign, it is remarkable that an

Sect. 2.1]

63

Curvilinear coordinates and metric tensor on a surface

inequality of Korn's type "on an elliptic surface" that only involves the linearized change of metric tensor in its right-hand side can be established (Thm. 2.7-3). This inequality asserts the existence of a constant CM such that

{

ll,oll + (:It

}1/,.

~/2 O~lf ~

for all ~ / - VM(W) -- H i ( w ) x H01(w) x L2(w). The existence and uniqueness of a solution to the two-dimensional equations of a linearly elastic elliptic membrane shell then foUow from this inequality. Note that Chaps. 1 and 2 together provide a unified presentation of inequalities of Korn's type "in curvilinear coordinates", whether in a three-dimensional domain in IR3 or on a surface in IRa, notably by showing that aU these inequalities of Korn's type hinge cruciaUy on the lemma of J.L. Lions recalled in Thm. 1.7-1 and on ad hoc infinitesimal rigid displacement lemmas. 2.1.

CURVILINEAR COORDINATES TENSOR ON A SURFACE

AND METRIC

In addition to the rules governing Latin indices that we set in Sect. 1.1, we henceforth require that Greek indices and exponents, except e and v and ~- in the notations 0v and Or, vary in the set {1, 2} and that the summation convention be systematically used in conjunction with these rules. For instance, "Ta/3(r/) = 0 in w" means "Tab(r/) = 0 in w for a, t3 = I, 2", the relation Oa(~Tia i) -- (r//3la -- balg~13)a/3 --k (~73la -4- b/3ar//3)a 3

means that 3

2

2 a3

i--1

for a = 1, 2, etc.

,~--1

,~--1

64

Inequalities of Korn's type on surfaces

[Ch. 2

Fig. 2.1-1: Curvilinear coordinates on a surface and covariant and conteavariant bases of the tangent plane. Let S = 0(~) be a surface in Cs. The two coordinates yx, y2 of y G ~ are the cuxvilinear coordinates of ~1 = O(y) E S. If they are linearly independent, the two vectors a,~(y) = O,~O(y), which are tangent to the coordinate lines passing through ~, form the covariant basis of the tangent plane to S at ~ = 0(y); the two vectors a~(y) defined by a~(y) 9at3(y ) = ~ form its contravariant basis. Let t h e r e be given as in Sect. 1.1 a real t h r e e - d i m e n s i o n a l affine E u c l i d e a n space s e q u i p p e d w i t h a Cartesian f r a m e consisting of a n origin O t o g e t h e r w i t h t h r e e vectors ~i _ ei forming a n o r t h o n o r m a l basis, a n d let a . b, lal, a n d a/x b denote the E u c l i d e a n inner p r o d u c t , the E u c l i d e a n n o r m , a n d the vector p r o d u c t of vectors a , b in t h e a s s o c i a t e d space E s. In a d d i t i o n , let there be given a t w o - d i m e n s i o n a l vector space, in w h i c h two vectors e a = e a form a basis; this space will accordingly be identified with I~2. We let ya denote the c o o r d i n a t e s of a p o i n t y in this space a n d we let Oa "= O/Oya a n d 0a~ := 02/OyaOy~. Finally, let t h e r e be given a d o m a i n w in ]R2 (according to the definition given at the b e g i n n i n g of Sect. 1.7) a n d an injective m a p p i n g

Sect. 2.1]

C u r v i l i n e a r coordinates a n d m e t r i c t e n s o r o n a surface

65

O" ~ --4 E 3. The set s :: is called a s u r f a c e in E 3. Each point 9 E S may thus be unambiguously written as 9 - o(y),

y e

and the two coordinates Ya of y are called the c u r v i l i n e a r c o o r d i n a t e s of ~ (Fig. 2.1-1). Well-known examples of surfaces and of curvilinear coordinates and their corresponding coordinate lines (defined below) are given in Figs. 2.1-2 and 2.1-3.

Remark. According to the usual terminology, the set 0(w) is a two-dimensional manifold, while the surface 0(~) is a two-dimensional manifold "with boundary", in E 3. By contrast, a two-dimensional manifold "without boundary" in E 3, such as a sphere or a torus, requires for its description several mappings Op 9wp C I~2 ---> E 3, p - 1, 2, . . . , P, satisfying ad hoc compatibility conditions on the "overlapping submanifolds" Op(wp) N Oq(wq), p ~ q, of S. Excellent (and particularly readable!) introductions to finitedimensional manifolds are given in Schwartz [1992, Chap. 3, Sect. 9], Schwartz [1993, Chap. VI, Sects. 8-10], and do Carmo [1994, Chaps. 3 and 4]. ll Naturally, once a surface S is defined as S = 0(~), there are infinitely many other ways of defining curvilinear coordinates on S, depending on how the domain w and the mapping 0 are chosen. For instance, a portion S of a sphere may be represented by means of Cartesian coordinates, spherical coordinates, or stereographic coordinates (Fig. 2.1-3). Incidentally, this example illustrates the variety of restrictions that have to be imposed on S according to which kind of curvilinear coordinates it is equipped with! Assume that the mapping O - 0 ~ ~ . w c R 2 -~ O(w) - S c E 3

is differentiable at a point y E ~. If r thus have 0(y +

- 0 ( y ) + v0(y)

is such that (y + r

y +

E ~, we

66

Inequalities of Korn's type on aurfaces

[Ch. 2

~d

Fig. 2.1-2: Two familiar ezamples of surfaces, curvilinear coordinates, and coordinate lines. A portion S of a circular cylinder of radius R corresponds to a mapping O of the form (~, ~) -~ (R~os ~, R ~ h ~ , ~). A portion S of a torus corresponds to a mapping 0 of the form (~, x) -~ ((R + . ~o~ x) ~o~ ~, (R + . ~o~ x) s i . ~, R s h ~), with R > r. In each case, the corresponding coordinate lines axe represented on S with self-explanatory graphical conventions; see also Ex. 2.1.

where the matrix V0(y) is given by

VO(y) .-

I OiOi 01030203 0~02

0202

/

(Y).

Sect. 2.1]

Gurvilinear coordinates and metric tensor on a surface

67

# sSss

sD

__2]

Fig. 2.1-3: Several systems of curvilineav coordinates on a sphere. Let ~ be a sphere of radius R. A portion S C ~ contained in the "northern hemisphere" can be represented by means of Cartesian coordinates: (~, y) -+ (~, y, { R ~ _ (~, + y~)}~/~). A portion S C ~ that excludes a neighborhood of both "poles ') and of a "meridian" (to fix ideas) can be represented by means of spherical coordinates: (~v, r --+ (R cos r cos ~v, R cos r sin ~, R sin r A portion S C ~ that excludes a neighborhood of the "North pole" can be represented by means of stereographic coordinates: ( 2R2u 2R2v u ~ + v 2 - R ~) (u, v) ~ u2 + v2 + R2 , u2 + v2 + R2 , Ru~ + v2 + R2 . As in Fig. 2.1-2, the corresponding coordinate lines are represented in each case with self-explanatory graphical conventions (see also Ex. 2.1).

68

Inequalities of Korn's type on surfaces

[Ch. 2

A w o r d of c a u t i o n . The presentation in this section follows t h a t of Sect. 1.2, "the mapping 8 9~ C It~2 -+ E 3 replacing the m a p p i n g O 9fl C R 3 --+ 6 3". As such, there are strong similarities between the two presentations, such as the way the metric tensor is defined in each case (see below), but there are also sharp differences. For instance, the matrix V 0 ( y ) is not a square matrix, while the m a t r i x VO(a~) is one! m Let the two vectors aa(y) E IR3 be defined by

a~(y) .= 0~o(y) -

IO~Oi1 0~02

(y),

0~03

so t h a t aa(y) is the a-th column vector of the matrix V 0 ( y ) . Let 5y - 5yaea; then the expansion of 8 about y may be also written as

o(y + ~y) = o(y) + 5y"~,(y) + o(~y). If in particular ~y is of the form ~y - r where ~t E IR and ea is one of the basis vectors in IR2 this relation reduces to

0(y + ~te~) = 0(y) + ~ t ~ ( y ) + o(~t). We henceforth assume that the two vectors aa(y) are linearly independent. The last relation thus shows that in this case each vector aa(y) is tangent to the a - t h c o o r d i n a t e line passing through 9 - 0(y), defined as the image by 8 of the points of ~ t h a t lie on a line parallel to ea passing through y; cf. Fig. 2.1-1 (there exist to and tl with to < tl and 0 E [to, tl] such that the equation of the a - t h coordinate line is t E [to, tl] --+ f a ( t ) :-- O(y + tea) i n a sufficiently small neighborhood of Y; hence :f~(0) - OaO(y) - aa(y)). The vectors aa(y), which thus span the tangent plane to the surface S at = 0(y), form the c o v a r i a n t b a s i s o f t h e t a n g e n t p l a n e to S at Y; cf. Fig. 2.1-1. Remark. A differentiable mapping 0 9~ C R 2 -4 R 3 such t h a t the two vectors OaO(y) are linearly independent at all points y E

Sect. 2 . 1 ]

Curvilinearcoordinates and metric tensor on a surface

is called an immersion.

69 B

Naturally, we are committing here two convenient abus de fangage: The vector tangent to the a - t h coordinate line at ~ - 8(y) is in fact the vector in the affine space t; 3 that is parallel to ha(y) and has ~ as its origin. Likewise, the tangent plane to S at ~ is in fact the aJ~fine plane in the affine space E ~ that passes through ~ and is parallel to the vectors ha(y). Returning to a general increment ~y = 5yaea, we also infer from the expansion of 0 about y that

le(y + ~y) - e(y)l ~ - ~ y T v e ( y ) r v e ( y ) ~ y = 5y~(y).

+ o(l~yl ~)

~,(y)hy~ + o(l~y12).

In other words, the principal part of the length between the points 0(y + ~y) and O(y) is {hyaaa(y). a~(y)~y~} 1/2. This observation suggests the introduction of the symmetric matrix (aa~(y)) of order two, whose elements

are called called the Note that ha(y) are

the e o v a r i a n t c o m p o n e n t s of the m e t r i c t e n s o r , also first f u n d a m e n t a l f o r m , of the surface S at ~ = 8(y). the matrix (aa~(y)) is positive definite since the vectors assumed to be linearly independent.

In the next theorem, we review the fundamental formulas expressing the area and length elements at a point ~ - 8(y) of the surface S in terms of the matrix (aa~(y)); see also Fig. 2.1-4.

Inequalities of Korn's type on surfaces

70

[Ch. 2

2.1-1. Let w be a domain in ~2, let 8 : -~ -q E 3 be a smooth enough and injective mapping such that the two vectors ha(y) -- OaS(y) are linearly independent at all points y e ~, and let Theorem

s

=

(a) The area element dS(~) at ~ = O(y) E S is given in terms of the area element dy at y E -~ by

where a(y) := det(aa~(y)) and aa~(y) = ha(y)" a~(y). (b) The length element d[(9) at 9 - e(y) e S is given by

Proof. The relation (a) between the area elements is well known. In particular, it can also be deduced from the relation between the area elements dr(~) and dF(x) given in Thm. 1.2-1 (b) by means of an ad hoc "three-dimensional extension" of the mapping 8; cf. Ex. 2.2. The expression of the length element in (b) simply recalls that d[(~) is by definition the principal part with respect to ~y - 5yaea of the length [O(y § ~y) - 8(y)], whose expression precisely leads to the introduction of the matrix (aa~(y)). m Remark. The (otherwise natural) notation da(9) for the area element at ~ - 0(y) is avoided as it bears too much resemblance with the customarily used notation a(y) for det(aa~(y)), m The relations in Thm. 2.1-1 are used for computing surface integrals and lengths on the surface S (Fig. 2.1-4): Let A be a dymeasurable subset of ~, let .4 "- O(A), and let ] " A ~ ~ be a dS-measurable function. Then

](9)

-/A(/o 0)(y)

Sect. 2 . 1 ]

C u r v i l i n e a r coordinates a n d m e t r i c t e n s o r o n a surface

,

~;

I

71

R

"

Fig. 2.1-4: Area and length elements on a surface. The elements dS(fl) and d[(fl) at ~l = O(y) E S are related to dy and 6 ! / b y means of the covariant components of the metric tensor of the surface S; cs Than. 2.1-1. The corresponding relations are used for computing the area of a surface .~ = 8 ( A ) C S and the length of a curve C = O(C) C S, where C = 3e(I) and I C R.

I n p a r t i c u l a r , t h e a r e a o f .~ is g i v e n b y

Consider next a curve i n t e r v a l in I~ a n d f

-

faea

C

-

~(I)

in ~ , w h e r e I is a c o m p a c t

9 I -+ ~ is a s m o o t h e n o u g h i n j e c t i v e

Inequalities of Korn's type on surfaces

72

[Ch. 2

mapping. Then the length of the curve C "- O(C) is given by

length C "-

I-~(0 o ~)(t)idt =

aaf3(~(t))-d~ (t)-d~ (t)dt.

Remark. The first fundamental form is also used for computing angles between coordinate lines; cf. Ex. 2.3. m Let 5~ denote the Kronecker symbol. Given a point y E ~, the

four relations

unambiguously define two linearly independent vectors ha(y) in the tangent plane, which form the e o n t r a v a r i a n t basis of t h e t a n g e n t p l a n e (Fig. 2.1-1). To see this, let a priori h a ( y ) = YaZ(y)a~(y) in the relations aa(y).a~(y) - 5~. This gives YaZ(y)a~(y) - 5~; hence ya~(y) = aa~(y), where (recall that the symmetric matrix (aa~(y)) is positive definite by assumption):

(aa[3(y)) :--(aa~(y)) -1. The elements aa~(y) of the symmetric matrix (aa~(y)) are called the c o n t r a v a r i a n t c o m p o n e n t s of the m e t r i c t e n s o r , or first f u n d a m e n t a l f o r m , of the surface S at ~ - 8(y). The relations a

(y) =

how t h a t

=

a"

(y)a

-

-

and thus the vectors aa(y) are linearly independent since the matrix (a af3 (y)) is positive definite. Let us assemble for convenience these fundamental relations between the vectors of the covariant and contravariant bases of the tangent plane and the covariant and contravariant components of the metric tensor" and and

Sect. 2.2]

2.2.

CURVATURE

C u r v a t u r e t e n s o r on a surface

TENSOR

73

ON A SURFACE

While a "three-dimensional manifold" in t; 3, i.e., a set O(~t) associated with a mapping 0 9~2 C I~3 -+ $~, is well defined by its "metric" (uniquely up to rigid deformations in 1t~3) provided ad hoc compatibility conditions are satisfied by the covariant components gij " ~t ~ IR of its metric tensor (Sect. 1.9), a "two-dimensional manifold" O(w) in t; a, i.e., a set O(w) associated with a mapping 0 9w c ~2 _+ E3, cannot be defined by its "metric" alone. We shall not dwell into this fascinating question in this section, referring instead to Fig. 2.2-1 for an intuitive example and to Thm. 2.8-1 for a precise statement. The "missing information" is provided by the "curvature" of the surface, introduced in this section by means of the covariant components of its curvature tensor. Consider as in Sect. 2.1 a surface S - 0(~) in t; 3, where the injective mapping 0 9 ~ C II~2 -+ t; 3 is smooth enough and such that, for each y E ~, the two vectors ha(y) - OaO(y) are linearly independent. For each y E ~, the vector

.

-

is thus well defined, has Euclidean norm one, and is normal to the surface S at the point 9 - O(y). This is another abus de langage as the vector normal to S at ~ is in fact the vector in the aJfine space t; 3 that has ~ as its origin and is parallel to ha(y). Note that the denominator in the definition of ha(y) may be also written as

where a(y) = d e t ( a ~ ( y ) ) (Sect. 2.1). This relation, which holds in fact even if a(y) - O, will be established in the proof of Thm. 2.5-1. Fix y C ~ and consider a plane P normal to S at ~ - O(y), i.e., a plane that "contains the vector a3(y)"; by the same abus de langage as above, "a plane containing a3(y)" means in fact any plane in the ajfine space ~3 that contains the point ~ and is parallel to the vector a3(y). The intersection C - P N S is thus a planar curve on S.

74

Inequalities of Korn's type on surfaces

[Ch. 2

i/ ! t

i/ I

t //

/7

iJ

Fig. 2.2-1: A metric does not define a surface in ~s. A flat surface So may be deformed into a portion $1 of a cylinder or a portion $2 of a cone without altering the length of any curve drawn on it (cylinders and cones are instances of "developable surfaces"). Yet it should be clear that in general So and Sz, or So and Sz, or $1 and $2, are not identical surfaces modulo a rigid deformation of R3!

As shown in Thm. 2.2-1, it is remarkable that the curvature of at ~ can be computed by means of the covariant components aa~(y) of the first fundamental form of S introduced in Sect. 2.1, together with the covariant components ba~(y) of the "second" fundamental ]orm of S; the definition of the c u r v a t u r e of a planar curve is recalled in Fig. 2.2-2. If the algebraic curvature of C at ~ is ~ 0, it can be written 1 as ~ , and R is then called the algebraic r a d i u s of c u r v a t u r e of the curve C at ~; this means that the c e n t e r of c u r v a t u r e of the curve C at ~ is the point (~)§ Ra3(y)); cf. Fig. 2.2-3. While R is

Curvature tensor on a surface

Sect. 2.2]

75

!

,

p(s).RvCs) \

p(s)

Fig. 2.2-2: Curvature of a planar curve. Let 7 be a smooth enough planar curve, parametrized by its curvilineax abscissa s. Consider two points p(s) and p(s + As) with curvilinear abscissae s and s + As and let Ar be the algebraic angle between the two normals v(s) and ~(s + As) (oriented in the usual way) to 7 at those points. When As ~ 0 the ratio Ar '

has a limit, called the "cuxvature"

A8

of 7 at p(s). If this limit is non-zero, its inverse R is called the (algebraic) "radius of curvature" of 7 at p(s) (the sign of R depends on the orientation chosen on 7). The point p(s) + Rv(s), which is intrinsically deft.ned, is called the "center of curvature" of 7 at p(s): It is the center of the "osculating circle" at p(s), i.e., the limit as As --~ 0 of the circle tangent to 7 at p(s) that passes through the point p(s + As). The center of curvature is also the limit as As ~ 0 of the intersection of the normals v(s) and v(s + As); consequently, the centers of curvature of 7 lie on a curve (dashed on the figure), called "la d~velopp~e" in French, that is tangent to the normals to 7.

not intrinsically defined (its sign changes in any system of curvilinear coordinates where "a3(y) is replaced by -a3(y)"), the center of curvature is intrinsically defined. If the curvature of C at ~ is 0, the radius of curvature of the curve C at ~ is said to be infinite; for this 1 reason, it is customary to still write the curvature as ~ in this case. 1 Note that the real number -R is always well defined by the formula given in the next theorem, since the symmetric matrix (aa~(y)) is positive definite. This implies in particular that the radius of curvature never vanishes along a surface S = 0(-~) defined by a mapping O

76

Inequalities of Korn's type on surfaces

[Ch. 2

satisfying the assumptions of the next theorem, hence in particular of class C2 on -~. It is intuitively clear that the vanishing of R implies t h a t 0 cannot be "too" smooth: Think of a surface made of two portions of planes intersecting along a segment, which thus constitutes a fold on the surface; or think of a surface O(~) with 0 E w and O(yl, y2) - ]yll l+a for some 0 < a < 1, so that 0 E c l ( ~ ; s but 0 ~ C2(~; s The radius of curvature of a curve corresponding to a constant y2 vanishes at yl - 0 . T h e o r e m 2.2-1. Let w be a domain in ~2 and let 0 E C2(~; s be an injective mapping such that the two vectors a a ( y ) = OaO(y) are linearly independent at all points y E -~. Fix y E -~ and consider a plane P normal to S = 0(-~) at the point ~1 - O(y). The intersection P A S is a curve C on S, which is the image C - O(C) of a curve C in the set-~. A s s u m e that the curve C is represented in a sufficiently small neighborhood of y as the image f ( I ) of a closed interval I C R with a non-empty interior, where ~ = f a e a : I --+ R is a smooth enough injective mapping that satisfies -~ dfa ( t ) e a ~ 0 where t E I is such that y - 5(t) (Fig. 2.2-3). 1 Then the curvature -R of the planar curve C at ~t is given by the ratio

1 R t)

where aa~(y) are the covariant components of the metric tensor of S at y (Sect. 2.1) and

Proof. (i) We first establish a well-known formula for the curva1 ture ~ of a planar curve. Using the notations of Fig. 2.2-2, we note that -

+

-

-{,.,(s

+

,.,(8)}.

+

Curvature tensor on a surface

Sect. 2.2]

Fig. 2.2-3:

77

Curvature on a surface.

al (y) A as(y)

Let P be a plane containing the vector 1 which is n o r m a l to S. T h e algebraic c u r v a t u r e ~ of t h e

p l a n a r curve C - P N S - O(C) at 9 -- O(y) is given by the ratio

R

~ , (r

dff'

dr:3.,

~t~

~ ,~)

dff3(.

where a~f3(y) a n d b,~(y) are the covariant c o m p o n e n t s of the m e t r i c a n d c u r v a t u r e tensors (also called the first a n d second f u n d a m e n t a l forms) of the surface S at ~9 a n d

(t) are the c o m p o n e n t s of the vector t a n g e n t to the curve

1 C - $t(I) at y = ~(t) - j:'~(t)e,~. If ~ r 0, the center of c u r v a t u r e of the curve (~ at t) is t h e point (!) + Raa(y)), E u c l i d e a n space C a .

which is intrinsically defined in the afFme

Inequalities of Korn's type on surfaces

78

[Ch. 2

so that 1 R

lim Ar ~.~o As

dr(s) ds

lim sin Ar h,-+o As

r(s).

(ii) The curve (8 o ~)(I), which is a priori parametrized by t E I, can be also parametrized by its curvilinear abscissa s in a neighborhood of the point ~. There thus exist an interval I C I and a mapping p - J -~ P, where J C I~ is an interval, such that

(0 o f)(t) - p ( s ) and (as o f)(t) - v(s) for all t e i, 8 e J, 1 By (i), the curvature ~ of C is given by 1

dv

-R =

ds (S) " r(s)'

where

dv (s) - d(az o f ) ( t ) d t dfdta dt d---s dt -~s = Oaa3(f(t)) (t) ds' dp d(O o f ) ( t ) d t r ( s ) - -~s(S)dt -~s df ~. dt ~~ dt = O~O(f(t))-~ (t)-~s = a~(f(t)) (t) d--~ Hence 1 _ R

(t)

(t) 1

To obtain the announced expression for ~ , it suffices to note that a,(f(t))

- b.,(I(t)),

by definition of the functions ba~ and that (Thm. 2.1-1)

dr. m

Remark. The knowledge of the curvatures of curves contained in planes normal to S suffices for computing the curvature of any

Sect. 2.2]

79

Curvature tensor on a surface

curve on S. More specifically, the radius of curvature/~ at 9 of any smooth enough curve C (planar or not) on the surface S is given by cos ~ = --,1 where ~ is the angle between the "principal normal" to R at 9 and a3(y) and ~ is given in Whm. 2.2-1; see, e.g., Stoker [1969, Chap. 4, Sect. 12].

II

Precise information about the shape of the surface in a neighborhood of its point ~ - 0(y) can thus be gathered by "letting the plane P turn around the normal vector a3(y)" and by following in this process the variations of the curvatures at ~ of the corresponding planar curves C - P N C, as given in Thm. 2.2-1. As we now show, these curvatures span a compact interval of R, i.e., they "stay away from infinity". 2.2-2. (a) Thm. 2.2-1. For a fixed normal to S at ~1 = O(y). planar curves P N S, P Theorem

[

]

Let the assumptions and notations be as in y E -~, consider the set 79 of all planes P Then the set of curvatures of the associated C 79, is a compact interval of I~, denoted

o=o of

bo h,

bo 0)

R~(y)' R~(y) (b) Let the matrix ( ~ ( y ) ) , a being the row index, be defined by

where (aa~(y)) - (aaf3(y)) -1 (Sect. 2.1) and the matrix (baf3(y)) is defined as in Thin. 2.2-1. Then 1

1

= b~(y) + hi(y), R2(y) det(ba~ (y)) 1 = b~(y)b~(y) b~(y)b~(y) d~t(~.~(y))" R~(y)R2(y)

R~(y)

t

1 1 (c) If R1 (y) ~ R2(y)' there is a unique pair of orthogonal planes P1 E 79 and P2 C 79 such that the curvatures of the associated planar 1 1

Inequalities of Korn's type on surfaces

80

[Ch. 2

Proof. (i) Let A ( P ) denote the intersection of P E T~ with the tangent plane to S at ~, and let (7(P) denote the intersection of P with the surface S; hence A ( P ) is tangent to (7(P) at ~ C S. Since we assume as in Thm. 2.2-1 that C ( P ) - (0 o S(P))(I) for some mapping f ( P ) : I C I~ --+ ~, the line A ( P ) is given by

A ( p ) --

~+

Ad(O o 5(P))(t); A e IR} dt

where ~a ._ dfa(P) (t) and ~aea # 0 by assumption. Since the line

"dt {y + tt~aea; t t e I~} is tangent to the curve C ( P ) " - 0 - 1 ( C ( P ) ) at

y E ~ (the mapping 8" ~ -+ R 3 is injective by assumption) for each such parametrizing function se(p) : I -+ C and the vectors as(y) are linearly independent, there exists a bijection between the set of all lines A ( P ) C T, P C 7~, and the set of all lines supporting the nonzero tangent vectors to the curve C(P). Hence Thm. 2.2-1 shows that when P varies in T', the curvature of the corresponding curves C ' - C'(P) at ~ takes the same values as does the ratio bal3(Y)~a~ when ~ "= (~a) varies in IR2 - {0}. (ii) Let the symmetric matrices A and B of order two be defined by

A "- (aa~(y)) and B := (baf3(y)). Since A is positive definite, it has a (unique) square root C, i.e., a symmetric positive definite matrix C such that A - C 2 (for a proof, see, e.g., Vol. I, Thm. 3.2-1). Hence the ratio

ba[3(Y)~a~[3 -- ~TB~ -- r / T C - 1 B C - l r / , where r / - C~,

is nothing but the Rayleigh quotient associated with the symmetric matrix C - 1 B C -1. When r/varies in I~2 - { 0 } , this Rayleigh quotient thus spans the compact interval of I~ whose end-points are the small1 1 est and largest eigenvalue, respectively denoted and

R (y)

of the matrix C - 1 B C -1 (for a proof, see, e.g., Ciarlet [1982, Thm. 1.3-1]). This proves (a).

Curvature tensor on a surface

Sect. 2.2]

81

Furthermore, the relation C ( C - 1 B C - 1 ) C -1 = B C -2 _ B A - 1 shows that the eigenvalues of the symmetric matrix C - 1 B C -1 coincide with those of the (non-symmetric in general) matrix B A -1. Note that B A -1 - ( ~ ( y ) ) with ~ ( y ) ' - a~(y)ba~(y), c~ being the row index, since A -1 - (aaf3(y)); hence the relations in (b) simply express that the sum and the product of the eigenvalues of the matrix B A -1 are respectively equal to its trace and to its determinant, det (baf3(y)) -1 _ which may be also written as since B A (b~a(y)). det (aaf3 (y)) This proves (b). (iii) Let rlz - (r]~) - C~z and r12 - (r~2) - C~2, with ~z - ((~) and ~2 - ((~), be two orthogonal (rlTrl2 -- 0) eigenvectors of the 1 symmetric matrix C - 1B C - z, corresponding to the eigenvalues

n (v)

1

and R2t)'y" respectively. Hence

o

-

-

-

-

o,

since C T - C. By (i), the corresponding lines A(P1) and A(P2) of the tangent plane are parallel to the vectors ~ a a ( y ) and ~af3(y), which are orthogonal since

{ ~ a a ( y ) }" {~fl2af3(y) } - aa/3(y)~fl2 - ~TA~ 2. 1 1 If RI(y) # R2(y)' the directions of the vectors rll and 7/2 are uniquely determined and the lines A(P1) and A(P2) are likewise uniquely determined. This proves (c). II We are now in a position to state several fundamental definitions: The elements ba~(y) of the (symmetric) matrix (ba~(y)) defined in Thm. 2.2-1 and the element ~ ( y ) of the (non-symmetric in general) matrix ( ~ ( y ) ) defined in Thm. 2.2-2 are respectively called the c o v a r i a n t c o m p o n e n t s and the m i x e d c o m p o n e n t s of the c u r v a t u r e t e n s o r , also called the s e c o n d f u n d a m e n t a l f o r m , of the surface S at ~ ) - O(y).

82

[Ch. 2

Inequalities of Korn's type on surfaces

A w o r d of c a u t i o n . With this definition of "curvature tensor", I depart from other texts~ where "Curvature tensor" of S often means the "Riemann curvature tensor" of S (the covariant components of this other tensor are defined in the last exercise of this chapter), m 1 1 The real numbers Ri(y) and R2(y) (one or both of which being possibly 0) found in Thm. 2.2-2 are called the p r i n c i p a l c u r v a t u r e s of S at ~. 1 1 If Ri(y) - R2(y)' the curvatures of the planar curves P N S are the same in all directions, i.e., for all P E P. If

1

R (y)

----

1

R (y)

-- 0,

1 1 the point ~ -- 8(y) is called a p l a n a r point; if (y---~ Ri - R2(y) ~ 0, ~) is called an u m b i l i c a l point; cf. Exs. 2.4 and 2.5. Let ~ - 8(y) E S be a point that is neither planar nor umbilical; in other words, the principal curvatures at ~ are not equal. Then the two orthogonal lines tangent to the planar curves Pi N S and P2 A S (Thin. 2.2-2 (c)) are called the p r i n c i p a l d i r e c t i o n s at ~. A line of c u r v a t u r e on S is a curve on S that is tangent to a principal direction at each one of its points. It can be shown that a point that is neither planar nor umbilical possesses a neighborhood where two orthogonal families of lines of curvature can be chosen as coordinate lines; see, e.g., Klingenberg [1973, Lemma 3.6.6]. If both

1

R (y)

and

1

R (y)

are ~ 0, the real numbers Ri(y) and

R2(y) are called the (algebraic) p r i n c i p a l r a d i i of c u r v a t u r e of 1 S at ~). If~ e.g., Ri(y) = 0, the corresponding principal radius of curvature Ri(y) is said to be infinite. While the principal radii of curvature may simultaneously change their signs in another system of curvilinear coordinates (as already noted), the associated centers of curvature are intrinsically defined. ( The numbers

1 Ri(y)

i ) t R2(y) and Ri(y)R2(y)' identified as

the principal invariants of the matrix ( ~ ( y ) ) in Thm. 2.2-1, are respectively called the m e a n c u r v a t u r e and the G a u s s i a n , or total~ c u r v a t u r e of S at ~.

Sect. 2.2]

Curvature tensor on a surface

83

As shown in Fig. 2.2-4, the points on a surface can be classified as elliptic, p a r a b o l i c , or h y p e r b o l i c , according as their Gaussian curvature is > 0, = 0 but they are not planar, or < 0. An a s y m p t o t i c line is a curve on a surface that is everywhere tangent to a direction along which the radius of curvature is infinite; any point along an asymptotic line is thus either parabolic or hyperbolic. It can be shown that, if all the points of a surface are hyperbolic, any point possesses a neighborhood where two intersecting ]amilies of asymptotic lines can be chosen as coordinate lines; see, e.g., Klingenberg [1973, Lemma 3.6.12]. As intuitively suggested at the beginning of this section, a surface in I~3 cannot be defined by its metric alone, i.e., by its first fundamental form alone, since its curvature must be in addition specified through its second fundamental form; see Sect. 2.8. But quite surprisingly, the Gaussian curvature can also be expressed solely in terms of the functions ha/3 and their derivatives! This is the celebrated Theorema egregium ("outstanding theorem") of Gautl [1828]; see Sect. 2.8. Another striking result where the Gaussian curvature is used is the equally celebrated Gaufl-Bonnet theorem, so named after Gaufl [1828] and Bonnet [1848] (for a "modern" proof, see, e.g., Klingenberg [1973, Tam. 6.3-5] or do Carmo [1994, Chap. 6, Tam. 1]): Let S be a smooth enough, "closed", "orientable", and compact surface in ~3 (a "closed" surface is one "without boundary", such as a sphere or a torus; "orientable" surfaces, which exclude for instance Klein bottles, are defined, e.g., in Klingenberg [1973, Sect. 5.5]) and let K : S --+ I~ denote its Gaussian curvature. Then K ( 9 ) dS(9) = 27r(2 - 2g(S)), where the g e n u s g(S) is the number of "holes" of S (for instance, a sphere has genus zero, while a torus has genus one; cf. Ex. 2.6). The integer X(S) defined by x ( S ) : = ( 2 - 2 g ( S ) ) i s the E u l e r c h a r a c t e r istic of S. A d e v e l o p a b l e s u r f a c e is one whose Gaussian curvature vanishes everywhere (this is the definition of Stoker [1969, Chap. 5, Sect. 2]; developable surfaces are otherwise often defined as "ruled" surfaces whose Gaussian curvature vanishes everywhere, as in, e.g.: Klingenberg [1973, Sect. 3.7]). A portion of a plane provides a first example, in fact the only one of a developable surface all points of

84

Inequalities of Korn's type on surfaces

[Ch. 2

f

Fig. 2.2-4: Different kinds of points on a surface. A point is elliptic if the Gaussian curvature is > 0 or equivalently, if the two principal radii of curvature are of the same sign; the surface is then locally on one side of" its tangent plane. A point is parabolic if exactly one of the two principal radii of curvature is in_Finite; the surface is again locally on one side of its tangent plane. A point is hyperbolic if the Gaussian curvature is < 0 or equivalently, if the two principal radii of curvature are of different signs; the surface then intersects its tangent plane along two curves.

Sect. 2 . 3 ]

Covariantderivatives and Christoffel symbols on a surface

85

which are planar (Ex. 2.4). Any developable surface all points of which are parabolic can be likewise fully described: It is either a portion of a cylinder, or a portion of a cone, or a portion of a surface spanned by the tangents to a skewed curve. The description of a developable surface comprising both planar and parabolic points is more subtle (although the above examples are in a sense the only ones possible, at least locally; see Stoker [1969, Chap. 5, Sects. 2 to 6]). The interest of developable surfaces is that they can be, at least locally, continuously "rolled out", or "developed" (hence their name), onto a plane without changing the metric of the intermediary surfaces in the process. Remarks. (1) That such "continuously varying isometric surfaces" exist plays a key r61e in the theory of "flexural shells" (Chaps. 6 and 10). (2) Interesting connections between the theory of developable surfaces and the appearance of folds on plates and shells subjected to applied forces have been exhibited and studied by Sanchez-Palencia [1995], Pomeau [1995], Ben Amar & Pomeau [1997]. II In Sect. 2.8, we shall briefly discuss the reciprocal question of recovering a surface 8(w) from its metric and curvature tensor fields: Given a positive definite symmetric matrix field (aa~) on w and a symmetric matrix field (ba~) on w, find conditions under which there exists a mapping 8 :w -+ t; 3 such that OaS" 0~8 = aa~ in w, O~e A 028 9 O a ~ 8 = ba~ in w.

Io o A o ol 2.3.

COVARIANT CHRISTOFFEL

DERIVATIVES SYMBOLS

AND

ON A SURFACE

The content of Sects. 2.1 and 2.2 and of the present section constitute our first encounter with differential geometry "on a surface". Other related notions are treated later, such as covariant derivatives of a tensor field on a surface (Thm. 2.5-1) and the recovery of a surface from its metric and curvature tensor fields (Sect. 2.8).

86

Inequalities of Korn's type on surfaces

[Ch. 2

For further details and complements, also for the notion of "tensots on a surface", see classical texts such as Valiron [1950, Chap. 13], Struik [1961], Stoker [1969], Klingenberg [1973], Spivak [1975], do Carmo [1976], or Berger & Gostiaux [1992, Chaps. 10 and 11] and the more recent books of do Carmo [1994] and Hsiung [1997]; Sanchez-Hubert & Sanchez-Palencia [1997] provide a wealth of complements particularly well adapted to shell theory. More "intrinsic" approaches to the differential geometry of surfaces have also been advocated in shell theory, notably by Destuynder [1990, Chap. 2], Podio-Guidugli [1991], Carrive [1995], Carrive,

TaUer

Mou o [1995], Valid [1995], Delfou

Zolts o [1997].

We begin by some definitions. As in Sects. 2.1 and 2.2, consider a surface S = 0(~) in E a, where 8 : ~ C R 2 --+ IRa is a smooth enough injective mapping such that the two vectors c a ( y ) - OaO(y) are linearly independent at all y C ~ and let

Then the vectors c a ( y ) (which form the covariant basis of the tangent plane to S at 9 - 0(y); see Fig. 2.1-1) together with the vector as(y) (which is normal to S and has Euclidean norm one) form the covariant basis at ~. Let the vectors c a ( y ) of the tangent plane to S at ~) be defined by the relations c a ( y ) 9af3(y) - ~ . Then the vectors c a ( y ) (which form the contravariant basis of the tangent plane at ~); see again Fig. 2.1-1) together with the vector a s (y) form the c o n t r a v a r i a n t basis at 9; cf. Fig. 2.3-1. Note that the vectors of the covariant and contravariant bases at 9 satisfy hi(y), aj (y) -- 5~. Consider an arbitrary d i s p l a c e m e n t field of the middle surface S, i.e., an arbitrary vector field ~ia i defined by means of its covaria n t components ~i " ~ -4 R; this means that ~Ti(y)ai(y) is the displacement of the point 9 = O(y) C S (Fig. 2.3-1). As we shaU see, finding the explicit forms of the associated linearized change of metric tensor (Thin. 2.4-1) and linearized change of curvature tensor (Thin. 2.5-1) requires the explicit forms of the

Sect. 2.3]

Covariant derivatives and Christof]el symbols on a surface

87



0

/

Fig. 2.3-1: Contravariant basis and displacement vector field along a surface. At each point ~ = O(y) E S, the thxee vectors ai(y), where a"(y) form the contravaxi-

~lCy) A ~,(y)

ant basis of the tangent plane to S at ~ (Fig. 2.1-1) and an(y) = lax(y ) A a2(y)l' form the contravariant basis at ~. An arbitrary displacement field of S may then be defined by its covariant components r/i : ~ --+ R: This means that ~7~(y)ai(y) is the displacement of the point ~. The mapping (0 + r/ia/) : ~ --+ gn defines a surface (0 + r/~ad)(5) in gn, which is thus equipped with the same cuxvilinear coordinates (the coordinates yl, y~ of y E ~) as those of the surface S = 0(~).

partial d e r i v a t i v e s Oa(~Tiai) of this vector field. These are found in the next theorem, as immediate consequences of two basic formulas, those of Gau~ and Weingarten. The Christoffel symbols "on a sur]ace" and the covariant derivatives "on a surface" are also naturally introduced in this process.

88

[Ch. 2

Inequalities of Korn's type on surfaces

Whenever no confusion should arise, we henceforth drop the explicit dependence on a particular point. For instance, the relation "Oaa 3 - - b a o a [3'' means that "Oaa3(y) - - b a o ( y ) a ~ ( y ) for all y E -~"; "Oaa 3 is in the tangent plane" means "Oaa3(y) is in the tangent plane to S at ~ - O(y) for all y C ~"; etc.

T h e o r e m 2.3-1. Let w be a domain in I~2 and let 0 E C2(~; s be an injective mapping such that the two vectors aa - OaO are linearly independent at all points of-~. (a) The derivatives of the vectors of the covariant and contravariant bases are given by the f o r m u l a s of Gauf$: 0~,

- r~,~

+ b~,~

and

O~a ~ -

~+

-r~

bl3aa3,

and Weingarten: Oaa3 - Oaa 3 - - b a o a [3 - - b ~ a a ,

where the covariant and mixed components bao and ~ of the curvature tensor of S are defined in Thms. 2.2-1 and 2.2-2 and r~.-

a ~ . o~ a~ - - o~ a ~ . a~ - r 3 ~

are the C h r i s t o f f e l s y m b o l s of the surface S. (b) Let there be given a vector field yia i with covariant components Yi E H i ( w ) . Then ~ia i E Hi(w) and the partial derivatives

0~(~)

~ ~2(~) ~

O ~ ( ~ a ~) -

g i ~ e . by

(0~

- r a[3~7~ ~ - ba/3~73)a/3+ (0a?']3 -~- bBa~/3)a3

-- (~7~]a - ba[3~73) ao -k (r/31a + b/3a~o)a3, where

tibia "-- 0a~//3 -F~O~/a and ~731a " - denote the f i r s t - o r d e r rlia i.

covariant

derivatives

OAT]3

of the vector field

Sect. 2.3]

Covariant derivatives and Christoffel symbols on a surface

89

P r o @ F i x a E {1, 2} throughout this proof. Since any vector c in the tangent plane can be expanded as c - (c-af3)a ~ - (c. a ~ ) a ~ , since Oaa 3 is in the tangent plane (Oaa 3 . a 3 - 8 9 3 -a 3) - 0), and since O a a 3 . a f ~ - -baf~ (Thm. 2.2-1), it follows that O a a 3 -- ( O a a 3 . a/3 )a/3 -- - b a / 3 a ~ ,

and thus the first formula of Weingarten is established. This formula, together with the definition of the functions ~ (Thm. 2.2-2), implies that o~a3 - ( o ~ a 3 . a ~ ) a ~ - - b ~ , ( a ~ . a ~ ) a ~ - - b ~ ~ ' ~ .

- -b;a~,

and thus the second formula of Weingarten is established. Any vector e can be expanded as e - (c. a i ) a i - ( e . a j ) a j. In particular, Oaaf3 -- (Oaa~o " a ~

. -~- ( O a a ~ " a 3 ) a 3

--

r ~ ~ + b~3,

by definition of F ~ all and bar3 Finally,

o.~

- (o.~'. ~)~

+ (0.~'. ~)~3 = _r~~

+ ~a3,

since O a a ~ . a 3 -- - - a ~ " O a a 3 -- b~acr " a ~ -

b/3a,

by the second formula of Weingarten; the formulas of Gaus are thus established. That rli a i C I-II(w) if rli C HI(w) is clear since a i C e l ( F ) if 0 E C2(~; E3). The formulas of Gaufl and Weingarten immediately lead to the announced expression o f Oa(~Tiai). m The definition of the covariant derivatives Ya[f3 - 0f3ya- F ~ "on a surface in C3'' given in Thm. 2.3-1 is highly reminiscent of the definition of the covariant derivatives Villi - 0ivi - r#vpP "in a threedimensional manifold in E ~'' given in Chap. 1. However, the former are more subtle to apprehend than the latter. To see this, recall that p the covariant derivatives villi - O j v i - F i j v p may be also defined by the relations (Thm. 1.4-1) ~

~llj~ ~ -

~

Oj(v~g').

90

[Ch. 2

Inequalities of Korn's type on surfaces

By contrast, even if only tangential vector fields ~Taaa on S are considered (i.e., vector fields yia z for which r/3 - 0), their covariant derivatives ~al/3 -- O ~ ? a - F 'ra~7~ only satisfy the more general relation ,

p

-

where P denotes the projection operator on the tangent plane in the direction of the normal vector (i.e., P ( c i a i) "= caaa), since -

+

3

for such tangential fields by Thm. 2.3-1. The reason behind this discrepancy is simple: While a "three-dimensional manifold in IR3'' has zero curvature (Sect. 1.9), a surface has in general a nonzero curvature, manifesting itself here by the "extra term" b~Taa 3. This term vanishes in ~ if S is a portion of a plane, since in this case b~ - ba~ - 0. Note that, again in this case, the formula giving the partial derivatives in Thm. 2.3-1 (b) reduces to =

We shall not dwell any further in this section into these aspects, referring instead to the references listed at the beginning of this section for more details. Meanwhile, the covariant derivatives Yila may be simply viewed as convenient notations. R e m a r k . The Christoffel symbols r ~

- a ~ . Oaa~ "on a surface

in d~3'' are to be carefully distinguished from the Christoffel symbols ri~ = g P ' O i g j "in a three-dimensional manifold in d~3'' introduced in Chap. 1. To avoid any confusion due to the identical notation when i, j, p E {1, 2}, specific notations shall always be introduced, should the two kinds of Christoffel symbols coexist in a given argument. II 2.4.

LINEARIZED CHANGE ON A SURFACE

OF METRIC

TENSOR

We recall that, given an arbitrary displacement field rig i of a three-dimensional manifold O(~) in E 3 defined by its covariant components vi 9 f~ --~ I~, the covariant components eillj(V) of the associated linearized change of metric tensor are defined by (see Thm.

Sect. 2.4]

Linearized change of metric tensor on a surface

91

1.5-1; also for the notations, not recalled here) 1 lin ~llJ(") - ~ [g~J(") - giJ] 9

It was then found that 1 e~llj(v) - ~(villj + vjlti ) = ~1 ( 0 j ~ + 0 ~ j )

- ri~vp.

Since a surface, i.e., a two-dimensional manifold in e s, also has a metric tensor (Sect. 2.1), it is natural to likewise define the covariant components of a "linearized change of metric tensor" associated with any displacement field defined on it; this is the object of this section. Notice the strong analogy between the next theorem and Thm. 1.5-1. T h e o r e m 2.4-1. Let w be a domain in R 2 and let 0 E C2(~; E a) be an injective mapping such that the two vectors aa = OaO are final A a 2 early independent at all points of-~, let as - la 1 A a2[' and let the vectors a i be defined by a i . a j = ~ . Given an arbitrary displacement field ~

of the surface S - 0(-~) with smooth enough covariant components ~li "-w --+ R, let the c o v a r i a n t c o m p o n e n t s of the l i n e a r i z e d c h a n g e of m e t r i c t e n s o r associated with this vector field be defined by

7~(~) .= ~1 [ ~ ( ~ ) - ~ ] lin where aaf3 and aa/3(Vl) are the covariant components of the metric tensor of the surfaces 8(~) and (0 + 71iai)(-~) (Fig. 2.3-1), and [... ]lin denotes the linear part with respect to ~ - (~i) in the expression [... ]. Then

1 1 - ~(rIalf3 -t- ~7/31a) - ba/3~73 1 = -~(o~, + o~)

- r ~ , 7 ~ - b~,Ts,

92

[Ch. 2

Inequalities of Korn's type on surfaces

where the Christoffel symbols F ~ and the covariant derivatives ~Tal~ are defined in Thin. 2.3-1 and the covariant components bad of the curvature tensor of S are defined in Thin. 2.2-1. Consequently,

r/a e Hi(w) and r/3 e L2(w) =~ 7af~(~7) e L2(w).

Proof. The covariant components aaf3(17) of the metric tensor of the surface (0 + yia')(-~) are by definition (Sect. 2.1) given by ao~(~) - o~(o + ~). o~(o +

#).

Note that both surfaces 0(~) and (0 + yiai)(-~) are thus equipped with the same curvilinear coordinates Ya. The relations

O~(o+#)=a~+O~# then show that a ~ ( ~ ) - (a~ + 0 ~ # ) . (a~ + 0~#) = aa/3 + O/3rl'aa + Oa*'l'af3 + OaO" 0/30,

hence that

7.z(n)

1

1

- ~ [ a o ~ ( n ) - aoz] "" - ~ ( 0 Z # 9~ . + 0 . 0 .

~Z).

The other expressions of 7of3(~7) immediately follow from the expression of 0a~/-- Oa(~Tiai) given in Thm. 2.3-1 (b). II While the expression of 7of3(r/) in terms of the covariant components rli of the displacement field is well known, that in terms of ~7 - ~?iaz seems to be less known; it was recently put to efficient use by Blouza & Le Dret [1994a, 1994b, 1999], who noticed that it has the advantage of still making sense under substantially weaker smoothness assumptions on the mapping 0; see Thms. 2.6-5 and 2.6-6. A w o r d of c a u t i o n . The vector fields ~/-- (~?i) and ~/=

~7ia*,

which are both defined on-~, must be carefully distinguished? While the latter has an intrinsic character, the former has not; it only provides a means of recovering the field ~/via its covariant components yi. II

Sect. 2.5]

2.5.

Linearized change of curvature tensor on a surface

93

LINEARIZED CHANGE OF CURVATURE TENSOR ON A SURFACE

As a surface S possesses a curvature tensor in addition to its metric tensor (Sect. 2.2), it is likewise natural to associate a "linearized change of curvature tensor" with any displacement field defined on S, through a process akin to that followed in Thm. 2.4-1 for defining the linearized change of metric tensor. Together, these two tensors play a major r~le in the theory of linearly elastic shells, as it shall be amply demonstrated in the next chapters. T h e o r e m 2.5-1. Let w be a domain in R 2 and let 0 E C3(~; s be an injective mapping such that the two vectors aa = OaO are linearly independent at all points of-~. Given a displacement field

of the surface S = 0(-~) with smooth enough and "small enough" covariant components 71i 9-~ -+ R, let the c o v a r i a n t c o m p o n e n t s of the l i n e a r i z e d c h a n g e of c u r v a t u r e t e n s o r associated with such a vector field be defined by

p.,(,)

:=

[ b . ~ ( , ) - b~,] "~,

where bar3 and bar3(rl) are the covariant components of the curvature tensors of the surfaces 0(-~) and (O+rliai)(-~) (Fig. 2.3-1), and [... ]tin denotes the linear part with respect to rI = (rli) in the expression [... ]. Then p.,(u)

= (0~

- r .~, 0 ~ )

9~3

p,.(u)

= v~l.~ - b ~ b ~ 3 + b~,~l~ + b~v.l. + b ~ l . ~ -" 0ctf~ ?73 -- r ~ f 30tr T]3 --

b~b~f3?73

94

Inequalities of Korn's type on surfaces

[Ch. 2

where the Christoffel symbols P ~ and the covariant derivatives ~lalf3 are defined as in Thm. 2.3-1,

Y31~ := Oa~r/3 - I'~130~7/3 and b~[a "- Oab~ +

- r x , b;

denote respectively a s e c o n d - o r d e r covariant d e r i v a t i v e of the vector field 7iia i and a f i r s t - o r d e r c o v a r i a n t d e r i v a t i v e of the curvature tensor of S, defined here by means of its mized components. Consequently,

71a e HZ(w) and r/3 E H2(w) =~ Pal3(~/) e L2(w).

The covariant derivatives br~[a satisfy the symmetry relations

Proof. For convenience, the proof is divided into five parts. In parts (i) and (ii), we establish elementary relations satisfied by the vectors ai and a i of the covariant and contravariant bases along S.

(i) The two vectors aa = OaO satisfy [al A a2l = v/-a, where a = det (ha/3). a l ((y)A y ) A a2(y) Let a3(y):= la a2(y)l and O(y, x3) :-- 8(y) + x3a3(y )

for

all y C ~ and z3 E I~. Using the notations of Sect. 1.2 (see notably Thm. 1.2-1), we have det V O = (gl A g2)'g3, where ga :-- Otto -- aa A- z3Octa3 and g3 :-- 0 3 0 = a 3 .

Assume for instance that det V O > 0 for Ix3] small enough, so that v/g - det V O for Ix3[ small enough, where g := det(gij) and gij := gi " gj. Hence V~[zs-O = d e t V O I z s = 0 = ( g l A g 2 ) ' g 3 [ z s - O = ( a l A a 2 ) . a 3 = t a l A a 2 ]

Sect. 2.5]

Linearized change of curvature tensor on a surface

95

on the one h a n d . Since

gl~3:0 - det

I gl'gl gl'g2 gl'g3 1 g2 gl g2"g2 g2"g3 g3 "gl g3 "g2 g3 "g3

a l . aall = det t a2

aa2.a2 l.a2 0

0

i~3=0

00 t 1

= det (aa~) - a on the other, the assertion is proved. T h e case where det V O for Ix31 small e n o u g h is t r e a t e d analogously.

< 0

(ii) The vectors ai and a a are related by al A a3 -- --v/aa 2 and a3/~ a2 - -v/-da 1. To prove t h a t two vectors c a n d d coincide, it suffices to prove t h a t c . a i - d . a i for i E {1, 2, 3}. In the present case, ( a l A a3) . a l = 0 a n d ( a l A a3) . a 3 = 0, (a~ A , ~ )

a~ 9 -

-(a~

A ,,~)

a~ 9 -

-v~,

since v/-da3 - a l A a2 by (i), on the one hand; on the other, -v~a~

9a l

-

-~a~

9a ~ -

o ~cl

since a i . a j - 5j. Hence a l A a3 similarly established.

- v~a~

9a ~ -

-~,

-~/-da 2. T h e other relation is

(iii) The covariant components ba~(~l) and ba~ satisfy bad(r/) - ba~ + ( 0 a ~ / -

F~0z~)

9a3 + h.o.t.,

where, here or in any other similar expansion found subsequently in this part of the proof, "h.o.t." stands for "terms of order higher than linear with respect to rI - (71i) ". Consequently, p~,(o)

:= [b~,(o)

- b o , ] ~'" -

(0o,~

- r;,0=~)

.~

-

p,o(o).

Since the vectors aa - Oa8 are linearly i n d e p e n d e n t in ~ a n d the fields r/ - (r]i) are s m o o t h enough by a s s u m p t i o n , the vectors

96

[Ch. 2

Inequalities of Korn's type on surfaces

Oa(O + ~Tia') are also linearly independent in ~ provided the fields are "small enough", e.g., with respect to the norm of the space C~(~; I~3). The following computations are therefore licit as they apply to a linearization around r / = 0. Let

as(r/) := Oa(8 + O) = aa + OaO and a3(r/):=

~(n) A a2(n)

where (cf. (i)) a(r/) '-- det(aaf~(r/)) and aa3(rl)"- aa(rl), afl(rl). Then

b~,(n) - o ~ , ( n ) . ~(n) 1 = --..~/a(17)(Oaafl + 0af3O)" (al A a2 + a l A 02~ + 01~ A a2 + h.o.t.)

1

= v/~(~) { ~(bo~ + oo~o. ~) } 1

+ v/~(n----5 { ( r o ~ + b o ~ ) . (~ A o~0 + o~0 A ~ ) + h.o.t.}, since bail - Oaafl.a3 and Oaafl - r ~afla~ + baf3a3 by the formula of Gaufl (Thm. 2.3-1 (a)). Next,

(r~a~ +

baf3a3). ( a l A ~20)

= r~,~. = ~

( ~ A o2~) - bo, O~O. (a~ A ~3)

( - r ~ o ~ o . ~ + bo~o~o. ~ ) ,

since, by (ii), a 2 . (al A 02~) -- - 0 2 ~ " (al A a2) -- - v ~ O 2 O . a 3 and a l A a3 - -v/-aa2; likewise,

( r 2 " ~ + b . ~ 3 ) . (o~0 A ~ ) - 4 ~ ( - r ~ , o ~ 0 . ~ + b.,o~n. ~). Consequently, bat3(r/) -

a a(r/) {bat3(1 + 0~0" a ~) + (0at30 - r ~ , o ~ ) 9~3 + h.o.t.}.

Sect. 2.5]

Linearized change of curvature tensor on a surface

97

There remains to find the linear term with respect to r/ - (r/i) 1 1 in the expansion v/a(,/) - ,/_d(1 + . . . ) . To this end, we use the Y

formule~ (see, e.g., Vol. I, Sect. 1.2) d e t ( A + H) - (det A)(1 + tr A - 1 H + o(H)), with A " - (aa~) and A + H : - (aa~(17)). In this case, H - ( O ~ O ' a a + OaO'a/3 + h.o.t.),

since [aa~(~) - a,~] fin -- O~O " aa + Oa~7 " a# (Thm. 2.4-1). Therefore, a(r/) - det(aa~(r/)) - det(aa~)(1 + 20aO" a a + h.o.t.), since A - 1 _ (aa~); consequently, 1

v/~(n)

1 ~(1-

O a i l . a a + h.o.t.).

Noting that there are no linear terms with respect to r/ - (yi) in the product ( 1 - OaO" aa)(1 + 0 ~ - a * ) , we find the announced expansion, viz., ba~(17) - ba~ + (Oa/30 - F ~ 0 ~ 0 )

9a3 + h.o.t.

(iv) The components pa~(rl) can be also written as

where the covariant derivatives ~731a/3 and br~]a are defined in the statem e n t o] the theorem.

By Thm. 2.3-1 (b),

0~

- (0~

- r ~ z ~ - b~,~3)~' + ( 0 ~ 3 + b ; ~ ) a 3.

Hence

since a i . a 3

-- ~ . Again by Thm. 2.3-1 (b),

Inequalities of K o r n ' s type on surfaces

98

o o , 0 . ~3 -

oo { ( o , ~

- r~.o~ - ~,~)~"

+(o,~3 + b~)~ = (0~

[Ch. 2

- r~~

}.~ - b,~3)Oo~.~

+(0~r/3 + b~7,)Oaa3.a3 = b~ ( o , ~ . - r ~ . , . )

- ~.,

~ + o.,~

+(0~b~),~ + b$0.,.,

since O a a ~ " a 3 -- ( - - r ~ r a Oaa 3 . a3 -

cr

r % baa

3

) . a3 -

cr

ba,

- b a ~ a ~ " a 3 -- O,

by the formulas of Gaug and Weingarten (Thm. 2.3-1 (a)). We thus obtain p~(r/) -

(0~0 - r~,~O~).a3

= b;(o,,. - r~,~)

- b~ba~3 + (gaf3rl3 + (Oab~)rlr + b~Oarlr

While this relation seemingly involves only the covariant derivatives Y31a~ and Yzl~, it may be easily rewritten so as to involve in addition the covariant derivatives Yrla and b~la. The stratagem simply consists in using the relation r ~ b ~ - r~b~ - 0! This gives Pot~ ( ~ )

--

(Ootl~ ?73 -- r~f3 (Or ?73 ) -- b~ b ~ ?73

+bX(oz~ - r~~)

+ b~(o~

- rx~n~)

(v) The covariant derivatives b~la are s y m m e t r i c with respect to the indices a and 13. Thanks to the formulas of Gaug and Weingarten (Thm. 2.3-1 (a)), we can write o - o o , ~ ~ - o , o ~ ~ = oo ( - r ~ ~ + b ~ ~) - o , ( - r : ~ ~ + b ~ ~) _- _ _ ( o o r ; ~ ) ~ ~ + ~r v - r ; ~ ba~ a ~ + (oob; )a 3 - b ; b o ~ ~ ~ ~ o .~~

Sect. 2.5] +(0,r~)~

Linearized change of curvature tensor on a surface ~ - r~r~.~.

+ r~b~

99

3 - (0,b~)~ 3 + b~b,~ ~

Consequently, o - (o~,~ ~ - o~~).

~

- oob~ - o , b ~ + r ~ b ~

- r~bX,

on the one hand. On the other, we immediately infer from the definition of the covariant derivatives b~l a that we also have

and thus the proof is complete.

m

Remarks. (1) Covariant derivatives basil~ can be likewise defined when the curvature tensor is defined by means of its covariant components ba~; see Ex. 2.7. (2) The functions ca~ := b~b~[3 - c~a appearing in the expression of Pat3 (r/) are the covariant components of the third fundamental f o r m of S. For details, see, e.g., Stoker [1969, p. 98] or Klingenberg [1973, p. 48]. (3) While the functions ba~(~/) are not always well defined (the vectors aa(y) must be linearly independent in ~), the functions pa~ (~/) are always well defined, m

While the expression of the components pat3 (r/) in terms of the covariant components r/i of the displacement field is fairly complicated but well known (see, e.g., Koiter [1970]), that in terms of ~ - yia i is remarkably simple but seems to be new. As its "linearized change of metric counterpart" (Thm. 2.4-1), it was efficiently put to use by Blouza & Le Dret [1994a, 1994b, 1999], who showed that its principal merit is to afford the definition of the components Pat3(r/) under substantially weaker regularity assumptions on the mapping 8; see Thms. 2.6-5 and 2.6-6. A w o r d of c a u t i o n . As already observed after Thm. 2.4-1, the vector fields r / - (r/i) and ~ / - yia ~, which are both defined on-~, must be carefully distinguished!

II

Inequalities of Kovn's type on surfaces

100

[Ch. 2

Remarks. (i) The symmetry Pa~ (rl) = P~a (rI) is an immediate consequence of the expression pa~(rl) - (Oa~O - F~OrO) "a3 found there. By contrast, deriving the same symmetry from the other expression of pa~(rl) requires proving first that the covariant derivatives b~! a are themselves symmetric with respect to the indices a and ~ (cf. part (v) of the proof of Thin. 2.5-1). While a proof of the symmetry b~l a = b~l~ is thus not essential here, it shall definitely be later in the proof of Thm. 2.6-2. (2) We assume that 8 E C3(~; E 3) in Thin. 2.5-1 (while we only assumed 0 E 62(~; E 3) in Thm. 2.4-1) in order that pa~(r/) C L2(w) if ~ / e Hi(w) x Hi(w) x H2(w) 9 The culprits are the functions b~la appearing in the functions pa/3(r/). As already noted, Blouza & Le Dret [1994a, 1994b, 1999] have shown that such regularity assumptions on 0 can be weakened if only the expressions of 7al3(r/) and pa/3(r/) in terms of the field ~ are considered. I

2.6.

I N E Q U A L I T I E S OF K O R N ' S T Y P E A N D INFINITESIMAL RIGID DISPLACEMENT LEMMA ON A GENERAL SURFACE

The two-dimensional Koiter equations for a linearly elastic shell, so named after Koiter [1970], take the following form: The unknowns are the covariant components ~i: K " ~ -'-4 I~ of the displacement field ~ie,K ai o f t h e middle surface S = 0(~) of the shell and r := (r ~,K) satisfies (0~ denotes the outer normal derivative operator along the boundary of w):

e

{n-

e

x

x

~7i - Ou~3 --0 on "[0}, f~ { caaf3ar' = f~ pi'e71iC'-ady for all r / - (~?i) E VK(W),

Sect. 2.6]

101

Inequalities of Korn's type on a general surface

where 3'0 is a subset of Ow with length 3'0 > 0, 2~ > 0 is the thickness of the shell, 4Ae#~

As + 2p ~

aa~a 'Tr + 2# e (a a'7af3"r + aara fh')

denote the contravariant components of the two-dimensional elasticity tensor of the shell ()t e and pe are the Lam~ constants of the elastic material constituting the shell), 7af3(r/) and pa/3(rl) denote the covariant components of the linearized change of metric and change of curvature tensors associated with a displacement field 71iai of S (Sects. 2.4 and 2.5; their definitions are recalled in Thm. 2.6-1 below), and the given functions pi,~ E L2(w) account for the applied forces; finally, the boundary conditions r/i = 0~7/3 = 0 on 3'0 express that the shell is clamped along the portion 0(3'0) of its middle surface (other boundary conditions are possible). These equations will be fully justified from three-dimensional linearized elasticity in Chap. 7, where various refinements and comments are also to be found. We shall later establish (Thm. 3.3-2) that there exists a constant ce = Ce(W, 0, p~) > 0 such that

Ita/3[2 < ceaa/3~r'e(y)t~rta~ a, f3

for all y existence means of existence

C~

_
0 such that

]~.~12 _< ~ ~ , ~ ( y ) ~ ~ a,~

for all y C ~ and all symmetric matrices (ta~) (Thm. 3.3-2). Establishing the existence and uniqueness of a solution to the above variational problem by means of the Laz-Milgram lemma thus amounts to proving the existence of a constant CM such that

{Ell oLi

w

--

{

O~w

fo~ ~n ,7 = ( ~ ) e v ~ ( ~ ) .

118

[Ch. 2

Inequalities of Korn's type on surfaces

The objective of this section, based on Ciarlet & Lods [1996a] and Ciarlet & Sanchez-Palencia [1996], is to find sufficient conditions (which, remarkably, turn out to be also necessary; cf. Thm. 2.7-4), essentially bearing on the "geometry" of the surface S, guaranteeing that such an "inequality of Korn's type" holds. It is also worth noticing that the justification alluded to above of these two-dimensional membrane shell equations from three-dimensional elasticity will be carried out under precisely the same assumptions on the geometry of S (Chap. 4). We follow the usual pattern, i.e., we begin by proving an inequality of Korn's type "without boundary condition", which in fact holds for "arbitrary" geometries, even though it only involves the linearized change of metric tensor. Everything has its price, however: The norm !1~73112,~appearing in the left-hand side of the "first" inequality of Korn's type on a general surface (Whm. 2.6-1) is now replaced by the norm lY310,~. T h e o r e m 2.7-1 (second i n e q u a l i t y of K o r n ' s t y p e " w i t h o u t b o u n d a r y c o n d i t i o n s " on a g e n e r a l surface). Let w be a domain in I~2 and let 0 E C2(~; s be an injective mapping such that the two vectors aa - OaO are linearly independent at all points of-~.

1

"1

IT

denote the covariant components of the linearized change of metric tensor associated with the displacement field rlia~ of the surface S - 0(-~). Then there ezists a constant c o - co(w, O) such that

a

i

a,t3

Proof. The proof is analogous to that of Thm. 2.6-1 and, for this reason, is only sketched; it relies on the following steps" First, the space wM( ) . - { . c c

Sect. 2.7]

Inequality of Korn's type on an elliptic surface

119

becomes a Hilbert space when it is equipped with the norm !1" I]M defined by

i

a,f3

Next, the two spaces WM(w) and H i ( w ) x H i ( w ) x L 2 ( w ) coincide, thanks again to the identities -

+

-

and to the lemma of J.L. Lions (Thm. 1.7-1). Finally, the closed graph theorem shows that the identity mapping from the space Hi(w) x Hi(w) x L2(w) equipped with the product norm y - (~?i) ~ { ~ a l]Yall2,~ + 177312,~}i/2 onto the space WM(w) equipped with I1" IIMwhas a continuous inverse. Hence the announced inequality holds, m The next step consists in identifying sufficient conditions affording the "elimination" of the norms ]Yil0,~ in the right-hand side of the above inequality of Korn's type. Whether it be for the threedimensional Korn inequality in curvilinear coordinates (Thm. 1.7-4) or for the inequality of Korn's type on a general surface (Thm. 2.6-4), the corresponding eliminations simply resulted from imposing ad hoc boundary conditions on the displacement fields. This idyllic scheme needs to be drastically amended in the present case! If we were following the same pattern, we would first prove an "infinitesimal rigid displacement lemma without boundary conditions", characterizing those displacement fields y~a z with covariant components Ya E Hi(w) and y3 E L2(w) that satisfy 7af3(Y)- 0 in w. The most powerful result in this direction is due to Blouza & Le Dret [1999, Thin. 6]: /f the three covariant components ~7~ of the displacement field are in L2(w) and V~f3(Y) - 0 in w, then there exists r E H - i (w) such that - r A 0

0.

However, this characterization does not provide an explicit form of the corresponding displacement field (compare with Thm. 2.6-3, or with Thm. 1.7-3 in the three-dimensional case); in fact it does

120

Inequalities of Korn's type on surfaces

[Ch. 2

not even allow to conclude that the space formed by such fields is finite-dimensional! We are thus left to directly establishing an "infinitesimal rigid displacement lemma with boundary conditions", i.e., to finding in particular boundary conditions guaranteeing that the semi-norm

.

(,,I

I o l.lr } a,f~

becomes a norm for the displacement fields ~7ia i that satisfy them. Since 773 is only in L2(w), the only choice consists in "trying" the boundary conditions ~?a = 0 on 70 C 7, with length 70 > 0. It then turns out that such an infinitesimal rigid displacement lemma does hold, but only for special geometries of the surface S and special subsets 0(70) of the "boundary" of S. We refer to Lods g~ Mardare [1998a], Mardare [1998c], and SUcaru [1998] who have identified various situations of interest where this lemma holds; such situations are described in Chaps. 4 and 5. Note in passing that such geometrical restrictions occur "for the first time" in our derivations of inequalities of Korn's type.

But the worst is yet to come! For, even though this infinitesimal rigid displacement lemma "often" holds, it "seldom" implies that the norm rl --+ {~a,f~ I')'afl(rl)12,o~}1/2 is equivalent to the product norm

n -

2

Ii, ll , + Jvsl0, ) More precisely, we shall see (Thm. 2.7-3) that, under ad hoc regularity assumptions on the mapping 0, these two norms are equivalent /f 7 = 70 and the surface S is "elliptic" according to the definition given below. In addition, Slicaru [1997] has shown the remarkable result that, even under "minimar' regularity assumptions, the same sufficient conditions are also necessary for the equivalence of these norms (see Thin. 2.7-4 for a more precise statement), which thus "seldom" occurs indeed! We begin by a fundamental definition: Let a surface S = 0(~) be given, where 0 E C2(~; E 3) is an injective mapping such that the two vectors a a -- OaO are linearly independent at all points of ~. Then S is elliptic if the symmetric matrix (baf3(y)) formed by the -+

Inequality of Korn's type on an elliptic surface

Sect. 2.7]

121

covariant components of the curvature tensor of S is positive, or negative, definite at all points y E ~; or equivalently if there exists a constant c such t h a t

I~a[ 2 < clba#(y)~a~#l for all y E ~ and all (~r

e R2

or equivalently if the Gaussian curvature of S (Sect. 2.2) is everywhere

strictly positive, i.e., if 1

R1 (y)R2(y) > 0 for all y E ~, where R~(y) and R2(y) are the principal radii of curvature of S at 8(y). A portion of an ellipsoid provides an instance of elliptic surface. In the next theorem, analytic functions of two real variables in an open subset of ]~2 a r e considered; we simply recall here their deftnition~ referring to Dieudonn~ [1968] for a particularly elegant treatment of analytic functions of any finite number of real or complex variables: Let w be an open subset of I~2; a function f : w -+ R is analytic if, given any y = (Yl, Y2) C w, there exists r > 0 and ainu E ~, m > O, n > O, such that the open ball of radius r centered at y is in w and OO

f(yl, m~ n - - 0

for all y' - (y~, y~) such that lY'-Y[ < r, these series being absolutely convergent. We also recaU t h a t a function belongs to the space C2'1(~) if it is in C2(~) and its second-order partial derivatives are Lipschit~continuous on ~. We now prove the announced "infinitesimal rigid displacement lemma", directly under the assumptions (70 = 7 and S is elliptic) t h a t will eventually lead to the equivalence of norms. For pedagogical purposes~ we assume in our proof more smoothness on the b o u n d a r y 7 and on the mapping 8 t h a n is necessary; in so doing, we essentially combine the proofs given by Ciarlet & Lods [1996a] and Ciarlet & Sanchez-Palencia [1996]. We refer to

122

[Ch. 2

Inequalities of Korn's type on surfaces

Lods & Mardare [1998a] for a proof under the more general assumptions stated in the theorem below. An earlier version of this lemma is due to Vekua [1962], who proved it under the assumptions that 7 is of class C3 and 0 E W3'P(w; Ea), p > 1, using the theory of "generalized analytic functions". T h e o r e m 2.7-2 ( i n f i n i t e s i m a l rigid d i s p l a c e m e n t l e m m a o n a n elliptic s u r f a c e ) . Let there be given a domain 03 in IR2 and an injective mapping 8 C C2'1(~; C 3) such that the two vectors aa - OaO are linearly independent at all points of-~ and such that the surface S : 0(-~) is elliptic. Then

n -- (r/i) E H i ( w ) • H i ( w ) • L2(w), ~ :ff ~ / _ 0 in 7af3(r/) - 0 in w

03.

J

Proof. We give the proof under the additional assumptions that the boundary 7 is of class C3 and that the components of the mapping 0 are restrictions to -~ of analytic ]unctions in an open set w' C R 2 containing -~.

(i) We first note that establishing this implication is equivalent to proving a uniqueness theorem, viz., ~7 = (vii) = 0 is the only solution in the space H i ( w ) x H i ( w ) • L2(w) of the linear system formed by the three partial differential equations 7af3(r/) = 0 in w together with the two boundary conditions (understood in the sense of traces) r/a - 0 on 7, or in eztenso, 01771 la2~i

--

+

i

r~l

T]a

0i~/2 -- r i ~ a 02,72 -

-

bll r/3 -- 0 in w,

-

bi2~a -

Oinw,

b22,/3 -

0 in w,

~r r22,/~ -

r]l

= 0ong,,

Y2

= 0onT.

(ii) A n y field n -- (77i) e Hlo(W) • H i ( w ) • L2(w) satisfying 7aft(Y) - 0 l a w and ya - 0 on 7 is in the spaceCt(-~)•215176 This regularity result relies on a crucial observation, due to Geymonat & Sanchez-Palencia [1991, 1995]: The partial differential equations 7af3(W) = 0 in w constitute a system, of the first order with

Inequality of Korn's type on an elliptic surface

Sect. 2.7]

123

respect to the functions ~?a and of order zero with respect to the function ~/3, that is "uniformly elliptic" in the sense of Agmon, Douglis & Nirenberg [1964]. This means that there exists a constant A > 0 such that (here and subsequently in this part of the proof, we use the notations of Agmon, Douglis & Nirenberg [1964]):

I ol < IL(y,

< A

(It

for all y E ~ and ~ = (~a) E R 2, where

~1 L(y, ~) := det

1

0

-bll(y)

1 9

0

~2

-b22(Y)

The way the above matrix of order three is constructed from the equations 7af3(r/) = 0 should be clear; suffice it to specify that only the coefficients of the partial derivatives of the highest order for each unknown (one for r/a and zero for ~73) are taken into account. The uniform ellipticity of the system "Taf3(v/) = 0 in w" thus holds since

L(y,

l~) - -

1

-~(~2 - ~I)

(

bii (y) b21(y) b22(Y)

~2

in the present case, and the symmetric matrix (baj(y)) is either positive, or negative, definite at all points y E ~ by the assumed ellipticity of S. In addition, the "supplementary condition on L " (which needs to be verified only in two dimensions, as here) is also satisfied: The degree m of the polynomial L with respect to ~1 and ~2 being two, the polynomial r E C ~ L(y, ~ § EC has exactly ~m _ one root T+ with Imv + > 0 for all y E ~ and all linearly independent vectors ~ - (~a) and v / - (r/a) in I~2. Finally, when ~one boundary condition, e.g., rh - 0 on 7, is appended to the equations "Taf3(v/) -- 0 in w', the "complementing boundary condition" is also satisfied: This means in this case that the polynomial r E C --+ ( T - T+) divides the polynomials T -+ c(~1 + T7/1) and r -+ c(~2 -4- r7/2) only if the constant c vanishes. ~Tt

__

124

[Ch. 2

Inequalities of Korn's type on surfaces

It then follows from Agmon, Douglis & Nirenberg [1964, Thm. 10.5] that, if-y is of class C3 and the coefficients of the uniformly elliptic system 3'a~(~/) - 0 are in the space C2(~), any solution r / E Hi(w) x Hi(w) • L2(w) of 3'a;3(r/) - 0 in w together with, e.g., 7/i = 0 on 3' is in the space HJ(w) x H J ( w ) xH2(w). The assertion then follows from the continuous imbeddings Hm(w) r cm-2(~), m > 2. (iii) Local uniqueness of the solution of "7a/3(~/) = 0 in w and ~la = 0 on 7 ". The assumed eUipticity of the surface S shows that there exists a constant c > 0 such that [btx(y)l _> c for all y E ~. Hence the unknown ~/3 may be eliminated by means of the equation 7ii (~/) - 0 (naturally, ~73 could be likewise eliminated by means of the equation 722(~/) = 0). This elimination shows that 1 Oll and that yi and 7/2 are solutions of the "reduced" system

b12 ( tr - 2 ~lt 0i 7/i + 027/i + 0i ~/2 - 2 ri2 - bi2 r~ri )7/~ -- O i n w , b22 01~1 + 02?72- (kr ~ 2 - b22r~ i ) ~ bii

-

0

in w,

~i -- O o n T , r/2 - 0 0 n T . Since the coefficients of this reduced system are analytic in w' and since the boundary 7 is of class C3 and is not a characteristic curve for this system, as is easily verified by using again the assumed ellipticity of the surface S, Holmgren's uniqueness theorem (see, e.g., Courant & Hilbert [1962, p. 238], Bers, John & Schechter [1964, p. 47], or Dautray & Lions [1984, Chap. 5, Sect. 1]) shows that "locally', i.e., in a small enough open neighborhood ~v C w' of any point of 7, (~/i, 7/2) = (0, 0) is the unique solution to this reduced system in ci(5~) x ci(&). Recalling that any solution T / - (7/i) of the "full" system is such that ~/a E c i ( ~ ) by (ii), we have thus shown: Any point of 7 possesses an open neighborhood ~v C w ~ such that the only solution 9/ - (7/i) E Hi(w) • Hi(w) x L2(w) of the "full" system "7a;3(~/) - 0 in w and Tla = O on T" is ~l = O in (v N-~.

Sect. 2.7]

Inequality of Korn's type on an elliptic surface

125

(iv) Global uniqueness of the solution of "Tab(r/) = 0 in w and 71a = 0 on 7 ' " By a theorem of Morrey & Nirenberg [1957], any solution of a u n i f o r m l y elliptic system whose coefficients are analytic in w is analytic in w. Since any solution ~/ = (7/i) of "Ta~(~/) = 0 in w and 7/a = 0 on 7" vanishes in a neighborhood of 7 by (iii) and ~ / = 0 is an analytic solution, the analytic continuation theorem for analytic functions of several variables (see, e.g., Dieudonn6 [1968, Thm. 9.4.2]) thus shows that r / = 0 is the only solution, m Several comments are in order about this theorem and its proof." As expected, the infinitesimal rigid displacement lemma is an "intrinsic" property of an elliptic surface" It also holds if the same surface is equipped with another system of curvilinear coordinates; cf. Ex. 2.11. The regularity theorem of Agmon, Douglis & Nirenberg [1964] used in part (ii) requires that only one boundary condition be added to the partial differential equations q'a~(~/) - 0 in w, but this boundary condition must be imposed on the entire boundary q,. Hence this analysis precludes the consideration of boundary conditions such as ~Ta - 0 on q'0 with length ~o < length V. A particularly interesting discussion about Holmgren's theorem and uniformly elliptic systems, especially adapted to linear shell theory, is given in Sanchez-Hubert & Sanchez-Palencia [1997, Chaps. 2 and 3]. We already mentioned that the regularity assumptions "8 analytic in w' D ~ and 7 of class C3'' can be substantially weakened. For instance, Ciarlet & Lods [1996a] assumed instead "0 E gs(~; E3) and 0' of class C4''. The analog of part (ii) in this case shows that the functions 7/1 and r/2 are in C2(~), again by resorting to the regularity theorem of Agmon, Douglis & Nirenberg [1964]; the "local uniqueness" of the solution 7/~ and r/2 of the reduced system (part (iii)) is then obtained by combining results of Carleman [1938] and Calder6n [1958] (by contrast with Holmgren's theorem, these results do not require the assumption of analyticity of the coefficients); finally, the "global uniqueness" (part (iv)) is obtained through the unique continuation theorem of Aronszajn [1956] applied to an elliptic equation satisfied by a single unknown, the auxiliary function (01~/2 - 0 2 r / l ) (also introduced in a different context by Bernadou, Ciarlet & Miara [1994]).

126

Inequalities of Korn's

type on

[Ch. 2

surfaces

The final word in this direction seems to have been achieved by Lods & Mardare [1998a] who were able to weaken the assumptions to those stated in Thm. 2.7-2, i.e., to "0 E C2'1(~; E 3) and V is Lipschitz-continuous". To this end, they notably made use of the unique continuation theorem of Hhrmander [1983]. In some special cases, Thm. 2.7-2 is easier to establish. For instance, an elegant and short proof, due to Brezzi [1994], applies to the special case where O(yl, y2) (Yl, Y2, f ( Y l , Y2)) (Ex. 2.12); as noted by Ciarlet & Lods [1996a], a portion of a sphere is likewise amenable to a simple proof (Ex. 2.13). It seems, however, that under the minimal regularity assumption "0 E C2(~; s all that can be proved is the finite-dimensionality of the space -

{,

=

e



-



0

This finite-dimensionality was established by Ciarlet & Lods [1996a], who reduced this issue to showing that the pair (YI, ~/2) belongs to the kernel of an operator of the form ( I - T), with T compact. As noted by Geymonat & Sanchez-Palencia [1991], this issue can also be resolved by resorting to Agmon, Douglis & Nirenberg [1964] or Geymonat [1965], under the assumptions "0 E C2(~; E 3) and ~' of class C 1". We are now in a position to prove the main result of this section, due to Ciarlet & Lods [1996a] and Ciarlet & Sanchez-Palencia [1996]; special mention must also be made of the early existence and uniqueness theorem for elliptic surfaces of Destuynder [1985, Thms. 6.1 and 6.5], obtained under the additional assumptions that the surface S can be covered by a single system of lines of curvature (Sect. 2.2) and that the C~ of the corresponding Christoffel symbols of S are small enough. In particular, Thm. 2.7-3 yields the ezistence and uniqueness of the solution to the two-dimensional equations of a linearly elastic membrane shell, as explained at the beginning of this section. The subscript " M " is appended to the constant as a reminder of this property. T h e o r e m 2.7-3 ( i n e q u a l i t y of K o r n ' s t y p e o n an elliptic surface). Let w be a domain in R 2 and let 0 E ~2,1(~; ~3) be an injective mapping such that the two vectors aa = OaO are linearly

Sect.2.7]

127

Inequality of Korn's type on an elliptic surface

independent at all points of-~ and such that the surface S elliptic. Given 0 - (m) ~ Hi(W) • Hi(W) • L2(w), let

0(-~) is

1

denote the covariant components of the linearized change of metric tensor associated with the displacement field rliai of the surface S. Then there ezists a constant CM = CM(W, O) such that

{

} 1/2 _< ,:M

I1oll Ol

for a11 ~ -

2 }1/2

~ I~(,)1o,,.,, a,fl

(~7i) C V M ( w ) " - H~(w) x H~(w)

x

L2(w).

Proof. (i) By the second inequality of Korn's type "without boundary conditions" on a general surface (Thm. 2.7-1), there exists a constant co such that

II,II~"c,,,)•215

:-

2 }I/2

I1~,~11~,,.,,+ I~lo,,,,

~

i

a,fl

for a11 U E Hi(w) • Hi(w) • L2(w) ~ VM(W). Hence it suffices to show that there exists a constant c such that

{

2}1/2

I~,1o,,., i

{

-< ,: ~ I~,~(.)lg,,,.,

}1/2 fo~ all n e VM(W).

a,/3

O0 (ii) If the last inequality is false, there exists a sequence (r/k)k_l of functions r/k --(y/k) e VM(w) such that

I Y~ 1~/~]0,~ 2) 1/2-

i

1 for all k and lim k ~ o o

IZ

211/2

lTat3(r/k)[0, ~

-0.

a,/3

In particular then, the sequence (r/k)~~ is bounded with respect to the norm [[ 9[[H~(~)•215 thanks again to the second inequality of Korn's type of Thm. 2.7-1. Since any bounded sequence in

128

[Ch. 2

Inequalities of Korn's type on surfaces

a Hilbert space contains a weakly convergent subsequence (see, e.g., Vol. I, Thm. 7.1-4), there exists a subsequence (~ll)~t and an element =

e

that

r/la ~ r/a in Hi(w) and rlla -+ Ya in L2(w), Y~ ~ Y3 in L2(w), where --~ and --+ denote weak and strong convergences (the compact imbedding H i ( w ) 9 L2(w) is also used here; see, e.g., Vol. I, Whm. 6.1-5).

(iii) Naturally, the difficulty rests with the subsequence (~/~)oo I:I which converges only weakly in L2(w). Our recourse for showing that it in fact strongly converges in L2(w) will be the assumed ellipticity of the surface S (see (iv)), but first, we prove that r / = (r/i) = 0. To this end, we simply note that yta ~ r/a in Hi(w) and yta ~ r/3 in L2(w) imply that 7~(r/l) ~ "ya;s(r/) in L2(w) on the one hand; since 7a~(n l) -+ 0 in L2(w)

on the other, we conclude that ~'afJ(~) : 0. Hence ~7 : 0 by Thm. 2.7-2. (iv) We next show that r]~ -+ 0 in L2(w). The strong convergences 7afj(~ l) -+ 0 in L2(w) and ,la --+ 0 in L2(w) combined with the definition of the functions 7af3(Y) imply the following strong convergences:

017"}~ -- b11,/3 -- {')'11(, I) d- F~I,~}

--+ 0 in L2(w), t --+ 0 in L 2 (w), 02~}I -Jr- 01./2 -- 2b12~7/3 -- {2")'12(r//) -4- 2F12r/,)

02?}/2 --b22,I -- {Q'22(, l) +

-+

0 i.

Since the function bll C C~ does not vanish in ~ by the assumed ellipticity of the surface S, we can eliminate 7/13between the first and second, and between the first and third, relations; this elimination yields"

{ 02 ?']i -~- 017}/2 -- 2

b12

522 1,02._ -- ~

0tr/~ } -+ 0 in L2(w)

Sect. 2.7]

129

Inequality of Korn's type on an elliptic surface

Multiplying the first relation by 02~?~and the second by 0z y~, then integrating over w, we get b12

{

I

l}

77102771

-

--~ 0,

~

since each sequence (Oa~7[)~z is bounded in L2(w) (each sequence even weakly converges to 0 in L2(w)). Subtracting the last two relations and using the relation f~ 02~?z01 ~72dy - f ~ 01~7102~72dy satisfied by all (~i,~72) E H~(w) x H~(w), we thus obtain + (511)2 (511522 - (512)

2

--~ 0.

Consequently, 0 1 ~ ~ 0 in L2(w),

since b11b22 -- (b12) 2 -- det(ba~) E C~ assumed ellipticity of S. Hence

does not vanish in ~ by the

(v) The relations ~ --~ 0 in L2(w) established in parts (iii) and (iv) thus contradict the relations { ~ , 1~?~12,~}1/2 - 1 for all I, and the proof is complete, m Finally, we state without proof a noteworthy result of Slicaru [1997, 1998], who showed that the sufficient conditions of Thm. 2.7-3 for obtaining an inequality of Korn's type (of the form given in this theorem) are also necessary! T h e o r e m 2.7-4. Let w be a domain in I~2, let 70 be a d 7measurable subset of V - Ow, and let 8 E C2(~; C3) be an injective mapping such that the two vectors a a -- Oa~ are linearly independent at all points of-~. Assume that there exists a constant c such that

z/2

}1/2 a,/3

130

Inequalities of Korn's type on surfaces

[Ch. 2

for all r / = (r/i) e V(w; 3'0), where

V(w; 70)"-- {T/-- (~7i) E H i ( w ) • HI(w) • L2(w); r/a -- 0 on ")'0} 9 Then "To = 7 and the surface S = 0(-~) is elliptic.

2.8 b.

m

COMPLEMENT: RECOVERY OF A SURFACE FROM ITS METRIC AND CURVATURE TENSOR FIELDS

The content of this section should be advantageously compared to that of Sect. 1.9. Let w be an open subset in ]R2 and let 8 : w -+ t; 3 be a thrice continuously differentiable mapping such that the two vectors aa = Oa8 are linearly independent everywhere in w. As before, let al Aa2 a3 = ]al A a21' let the three vectors a i be defined by the relations a J . a i - 5~, let aa[3 - aa "a/3 and ba[3 - a3" O/3aa, and let the Christoffel symbols be defined by r~a/3 = a ~ . O/3aa. In addition, let the Christoffel symbols of the first kind F a i r be defined by

r o , . := aarr~. In this context, the functions r ~ at3 are also called the Christoffel symbols of the second kind. Then it can be shown that the Christoffel symbols and the covariant components of the curvature tensor satisfy the following compatibility conditions (Ex. 2.14): 0~r.~

- 0~ro~ + r"~.r~, - r~.r~.~ O ~ b ~ - O~bo. + r ~ b ~

- r~.b~

- b . . b , ~ - b . ~ b , ~ i~ ~ , -

0 ~ ~.

These conditions are in effect relations between partial derivatives of the first, second, and third order of the mapping O. They are also relations between the covariant components aa~ and ba/3 of the metric and curvature tensors and their derivatives, since the Christoffel symbols r~t3r may be directly defined in terms of the functions aat3 as (Ex. 2.14): r~

1 - ~(~~

+ o~~

- o~~).

Recovery of a surface

Sect. 2.8 b]

131

R e m a r k a b l y , these necessary conditions are also sufficient for the existence of a m a p p i n g 0 :w C I~2 -+ E 3 whose metric a n d c u r v a t u r e tensor fields are given on w:

T h e o r e m 2.8-1. Let w be a simply connected open subset of R 2, and let there be given a twice continuously differentiable, symmetric, and positive definite matrix field (aa/3) on w and a continuously differentiable symmetric matrix field (ba[3) on w that together satisfy

-

O~ba# - Of3baa + r ~ b ~ :=

:=

- b,~b~r - b,~rb~ in w,

-

1

+

- r~b~

-

0 in w, where

-

:=

Then there exists a mapping O E C3(w; IR3) such that 0 a 0 " 0f30 = aaf3 in w,

0~o A 020 90af3O = bar3 in w. 10~o A 0201 Furthermore, this mapping is unique "up to rigid deformations in I~3 ": This means that any other solution is necessarily of the form y E w --+ c + Q 0 ( y ) , where e is a vector in IR3 and Q is an orthogonal matrix of order three. II For a direct p r o o f of this delicate result, see Klingenberg [1973, Thin. 3.8.8]. Otherwise, Thin. 2.8-1 can be also obtained as a corollary to Thin. 1.9-1; see Ciarlet & L a r s o n n e u r [2000]. T h e first relations constitute one version of the "Theorema egreg i u m " of Gaufl [1828] (Ex. 2.14), while the second ones are equivalent to the "Codazzi-Mainardi identities" (Ex. 2.7).

Inequalities of Korn's type on surfaces

132

[Ch. 2

EXERCISES

2.1. (1) Compute the vectors of the covariant and contravariant bases, the area and length elements, the Christoffel symbols, the covariant and contravariant components of the metric tensor, and the covariant and mixed components of the curvature tensor corresponding to a portion of a circular cylinder and to a portion of a torus equipped with the curvilinear coordinates shown in Fig. 2.1-2. (2) Carry out the same computations for a portion of a sphere equipped with the three kinds of curvilinear coordinates shown in Fig. 2.1-3. (3) In each case considered in (2), verify that the radius of the sphere indeed satisfies the relation established in Thm. 2.2-1. (4) Carry out the same computations as in (1) for a portion of a hyperbolic paraboloid represented by a mapping of the form

(~, y)-~ (~, y,

h

y),

where a, b, and h are three given lengths. 2.2. Show that the relation dS(~l) = v/a(Y)dy providing the area element at ~) = 8(y) e S = 8(~) (Thm. 2.1-1) can be recovered from the relation (Thm. 1.2-1)

aT(~)- ICofVO(x)n(x)ldr(x)

at ~ - O(x) e ~ - o(r),

by specializingthe mapping | to be the canonical extension of the mapping 8 (Thin. 3.1-1). 2.3. The notations and assumptions are as in Sect. 2.1. Let y E ~ be given. Show that the angle a(y) between the coordinate lines passing through the point O(y) satisfies cos a(y)

=

{~ (y)~2~(y))~/~"

2.4. Let the assumptions and notations be as in Thm. 2.2-1. A 1 1 point O(y) E S is called a planar point if R1 (y) - R2(y) = 0. Show that, if all the points of S are planar, S is a portion of a plane. Hint: See, e.g., Stoker [1969, p. 87].

Ezercises

133

2.5. Let the assumptions and notations be as in Thin. 2.2-1 and assume in addition that 0 E C3(~; E3). A point O(y) e S is called an 1 1 umbilical point if Rt (y) -- R2(y) ~ 0. Show that, if all the points of S are umbilical, S is a portion of a sphere. Hint: See, e.g., Stoker [1969, p. 99]. 2.6. Let K : S -+ IR denote the Gaussian curvature of a (smooth enough) surface S. (1) Let S be a sphere; show that fs g(~/)dS(~/) = 47r. (2) Let S be a torus; show that fs g(~/)dS(~/) = O. Remark. These are instances of applications of the Gaufl-Bonnet theorem (Sect. 2.2). 2.7. Let ba~l~ :-- O~ba~ - r [ ~ b ~ - r ~ b ~ denote the first-order covariant derivatives of the curvature tensor, defined here by means of its covariant components. Show that these covariant derivatives satisfy the Codazzi-Mainardi identities

which are themselves equivalent to the relations (Thm. 2.8-1) 0.bo,

- 0,bo~ + r;,b~

- r;~b~,

- 0.

Hint: The proof is analogous to that given in Thm. 2.5-1 for establishing the relations b~la - b~l#. 2.8. Let the assumptions on the mapping O be as in Thm. 2.6-3. (1) Let there be given ~/ - (7}i) e Hi(w) such that 3'a#(~/) - 0 in w. Show that

o~(~ia i)

-

r A o~o,

where

10~

with~tl-s22-O s t 2-_~ ,1 ,

ands2t-

1 ~.

Remark. The vector field ~ is the infinitesimal rotation field, introduced by Vekua [1962], then put to various uses by Bernadou & Ciarlet [1976, Lemma 2.5], Choi [1993], Choi & Sanchez-Palencia [1993]. Its existence under minimal regularity assumptions is established by Blouza & Le Dret [1999, Thm. 6].

134

[Ch. 2

Inequalities of Korn's type on surface8

(2) Let there be given rl - (r/i) E Hi(w) x Hi(w) x H2(w) such that 7aft(r/) -- Pat3(r/) - 0 in w. Show that the vector field r found in (1) is constant in this case and equal to the vector t/found in Thm. 2.6-3 (a). 2.9. Let the assumptions on the mapping 0 be as in Thm. 2.6-3 and let 70 be a relatively open subset of 7 that satisfies length "ro > O. (1) Show that the implication (the analog of Thm. 2.6-3 (b) for another class of boundary conditions):

~i - - 0 on 70,

=~ r / - 0 i n w

"Ya/J(r/) - Pa/3(~/) - 0 in w holds if and only if 0(70) is not a subset of a straight line. Hint: One way to solve this problem is to combine Thm. 2.6-3 (a) with Ex. 2.8. (2) Assuming that the implication of (1) holds, show that an inequality of Korn's type on a general surface analogous to that of Thm. 2.6-4 holds, where the space

v~c(~) := {. - (~) e H ~ ( ~ ) x H~(~) x H~(~); ~ = 0 on 70) replaces the space V g ( w ) found in ibid. The exponent "s" reminds that the space V}c(w ) corresponds to a shell that is simply supported along the curve 0(70), i.e., whose displacement field ~ia i satisfies the two-dimensional boundary conditions of simple support r - 0 on "y0. 2.10. (1) The notations and assumptions are the same as in Thm. 2.6-6. Show that the space V g ( w ) becomes a Hilbert space when it is equipped with the norm --+

]lOii2,~, + ~

10at3~/" a3]0,o,

9

a,/3

(2) Assume in addition that 0 E W3'~176 E3). Show that the mapping r / - (7/i) --+ ~ - 71iaz is an isomorphism between the space

v~(~)

.

-

H~ (~) • g~ (~) • {H ~(~) n H~(~)),

equipped with the product norm r/ --4 { ~ a IIr/a[[2,~ + IIr/sl]2,oJ}1/2, and the space ~'g(W) equipped with the norm of (1). Remark. This observation is due to Blouza & Le Dret [1999, Lemma 4].

Ezercises

135

2.11. Let an elliptic surface be equipped with two different systems of curvilinear coordinates. Show that, if the infinitesimal rigid displacement lemma on an elliptic surface (Thm. 2.7-2) holds for one system, it holds for the other. 2.12. Let w C I~2 be a domain with a boundary of class C2. (1) Let there be given functions Aaf3 E Ct(~) satisfying the following "ellipticity condition": There exists a constant c > 0 such that

Aa~(y)~a~ ~ ~ c ~

I~a[2 for aU y e ~ and all (~a) e R 2.

a

Show that, if X e H~(w) satisfies Aa~Oa~X e L2(w), then X e H2(w). Hint: Indications may be found, e.g., in Brezis [1983, Sect. 9.6]. (2) Let S = 8(~) be an elliptic surface with a mapping 8 of the

fo~m e - (y~, y~) e ~ ~ (y~, y~, f(y~, y~)), where f e C3(~). Show that a field v / - (v/i) e Hi(w) x Ht(w) x L2(w) satisfies 7af~(v/) - 0 in w if and only if there exists g C L2(w) such that 1

~ . z ( n ) . - ~(oz,~. + o.,~z) - g o . z f . (3) Show that, for all 7/a e H~(w) and all X E H~(w)N H2(w),

L

{ell (v/)022X - 2e12(~l)O12X + e22(~l)OllX} dy = O.

(4) Show that, if v/C H~(w) • H~(w) • L2(w) satisfies 7a/3(v/) - 0 in w, then v / - 0 in w. Remark. This result, which is due to Brezzi [1994], thus provides a considerable simplification of the proof of Thm. 2.7-2 for the special class of elliptic surfaces considered in (2). 2.13. Let S be a portion of a sphere with radius R, equipped with stereographic coordinates u and v (Fig. 2.1-3). Given any element

- (~) e H~(~) • H~(~) • L2(~), l~t Xa :-- rla(u2 -4- v 2 -4- R2) 2. Show that the relations 3'a/3(v/) = 0 in w imply that 02X1 -~-

O1X2 =

0 and

02X2 -

01X1 = 0 i n

w,

Inequalities of Korn's type on surfaces

136

[Ch. 2

and conclude in this fashion that 7/a = 0 in w, thus providing in this case a quick proof of Thm. 2.7-2 (this observation is found in Ciarlet & Lods [1996a, Sect. 3]). 2 914 9 (1) The Christoffel symbols are defined as r ctl3 ~ - a ~ . O~aa in the text (Thm. 2.3-1), i.e., by means of the vectors of the covariant and contravariant bases of the tangent plane. It is remarkable that they can be also defined solely in terms of the metric tensor of the surface. More precisely, show that r~

- ~ro~,

1 where r o ~ . - ~ ( 0 ~ ~

+ 0~~

- 0~a~).

(2) Show that the Christoffel symbols satisfy the compatibility conditions o~ro~ - o~ro~ + r"~r~.

- r~r~

0~boz - 0 z b ~

- bo~b~ - bo~b~ i~ ~,

+ rxzb,~ - r~b~z

- 0 in

w.

(3) ~ t R~

:= 0 ~ r ~

- o~ro~ + r.~r~.

- r~r~.

Show that R~

= -R~~

Raj311 = RaD22

= -R~~ -- Rlltrr

-

= R~, R22~rr --0,

R1212 = R2121 =-R1221 =-R2112, and that, consequently, the compatibility conditions found in (2) in fact reduce to R 1 2 1 2 - - bllb22 - - ( b 1 2 ) 2 . (4) Deduce from (3) that the Gaussian curvature K (Sect. 2.2) satisfies K - (alia22 - ( a 1 2 ) 2 ) -1 (02rl12 - 01r122 + r ~"r ~ .

- r ~ l r 22~).

This is the astonishing T h e o r e m a egregium of Gaul] [1828]: The Gaussian curvature depends only on the knowledge of the f i r s t fundamental form of a surface, i.e., only on its metric! R e m a r k . The functions Radar are the covariant components of the R i e m a n n c u r v a t u r e t e n s o r of the surface.

CHAPTER 3 ASYMPTOTIC ANALYSIS SHELLS: PRELIMINARIES

OF LINEARLY ELASTIC AND OUTLINE

INTRODUCTION

The purpose of this chapter is twofold: First and foremost, it gathers the fundamental preliminaries needed in the remainder of this volume for carrying out the asymptotic analysis of all the kinds of linearly elastic shells that we shall encounter: After ad hoc "scalings" of the unknowns (the covariant components of the displacement field) and ad hoc "asymptotic" assumptions on the data (the Lam6 constants and applied force densities) have been made, we transform the problem of a linearly elastic clamped shell with thickness 2e > 0 into a "scaled problem", defined over a domain that is independent ore. Second, it justifies the two fundamentally distinct classes of twodimensional equations that mathematically model linearly elastic shells~ through a formal asymptotic analysis of the solution of the scaled problems, where e is considered as the "small" parameter. Since this formal analysis will be later replaced by the more satisfactory (but also considerably more delicate) convergence theorems of the next three chapters~ this chapter thus essentially serves a pedagogical purpose. More specifically, let w be a domain in I~2 with boundary ~/and let ~ 9~ --~ 1~3 be a smooth enough injective mapping such that the two vectors aa : 0aS are linearly independent at all points in ~. Consider a shell with middle surface S = 8(~) and thickness 2e > 0, i.e., a body whose reference configuration is the set O ( ~ ) , where :,.,.,x]

-

O(x ~) - e ( y ) + xga3(y) for all x e - (y, xg) - (x~) e ~ , and a3(y) is the unit outer vector normal to S at #(y) constructed as in Sect. 2.2.

Asymptotic analysis of linearly elastic shells: Outline

138

[Ch. 3

The shell is subjected to applied body forces with contravariant components f/' ~ 9f~e -+ I~ and is subjected to a boundary condition of place along a portion (9(70 • I - e , el) of its lateral face (9(7 • I - e , e]), where 70 C 7 and length 70 > 0. Applied surface forces acting on the upper and lower faces O(w • {e}) and O(w x { - e } ) may be also considered; for simplicity, we assume in this introduction t h a t they vanish. Let )~e a n d / z e denote the Lam6 constants of the elastic material constituting the shell. T h e n in linearized elasticity, the unknown u ~ - (u~), where ui -+ R are the covariant components of the displacement field of the points of the shell, satisfies the following three-dimensional equations in terms of the "natural" curvilinear coordinates x i of the shell (we quickly review in Sect. 3.1 the main features of this variational problem, otherwise extensively studied in Chap. 1):

~," e v ( n ' ) -

{,," - ( W ) e I-I~(n'); ,, e = 0 on 3'0 x [ - e , e]},

fft AiJkl'ee~lll(ue)e~llj(Ve)~ dx e c

--

f n fi, eV ie v / ~ dz ~ for all v e E V(f~6), g

where

Aijkl, e = Ae gij, egkl, e + #~ (gik, egjl, e + git, egjk, e) , e~ (v ~

1

Ve

p, e

illJ -- O~v~ - r i j

V~.

In Sect. 3.2, we transform this problem into an equivalent problem, but now posed over the set ft = w x ] - 1, 1[, which is independent of e. This transformation relies in a crucial way on appropriate scalo ings of the unknowns u ie and assumptions on the data )t e, #~ and fz, ~. More specifically, we define the scaled unknown u(e) = (ui(e)) by letting

=~(~)

-

= ~ ( ~ ) ( ~ ) fo~ a n ~

-

~

e

~,

where lre(Zl, z2, x3) = (Zl, x2, ez3). We then assume t h a t there exist constants A > O, # > 0 and functions fi independent of e such that ~e = % and #e = #, i~,~(~~) - ~y~(~) fo~ an ~ - ~

E n~,

Introduction

139

where the exponent p is unspecified at this stage. It is found in this fashion that the scaled unknown u(e) satisfies a variational problem of the form (Thm. 3.2-1):

u(e) E V(ft) -- {v -- (vi) e H l ( f t ) ; v - 0 on 70 • [ - 1 , 1]}, f

AiJkl(e)eklll(e; u(e))eillj(e; v)v/g(e)dz

-- ~P ffl fivi v/g(e) dx for all v e V(ft), where, for any vector field v = (vi) E H l ( f t ) , the scaled linearized strains eillJ(S; v) -- ejlli(e; v) E L2(f~) are defined by:

1

-

eatlz(e;v) e3113(e; v )

p

-

l(103va+Oav3)

~ e u

--

+

-

e103v 3.

The specific form of this variational problem suggests that we use the method of formal asymptotic ezpansions, i.e., we let U ( g ) -- U 0 -~- g U 1 -~- S2U 2 -+- g3U3 q- g4U4 -+- " ' " , w i t h

u ~ ~ 0,

in the variational equations, and then we equate to zero the factors of the successive powers of e found in the resulting equations until the leading t e r m u ~ can be fully identified, without imposing any restriction on the applied force densities. In so doing, we are led after a series of delicate computations (which themselves rely on various "geometrical" and "mechanical" preliminaries established in Sect. 3.3) to the conclusion that the leading t e r m u ~ satisfies a two-dimensional problem that falls in one of the following two categories: Assume first that the space Vo(w) "- {W E Hi(w); r/- 0 on 7o, 7a/3(W) - 0 in w}

contains only the function 17 = O. Then the functions fi, e m u s t be of the form

fi'e(xe)

-- fi'O(x) for all x ~ - 7 r ~ x C ~Y,

140

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

where the functions f i , 0 a r e independent of e (i.e., the exponent p must be set equal to 0 in this case). Furthermore, the leading

term u ~ 9 -+ I~3 is independent of the transverse variable x3 and ~o _- 12f1-1 u~ dx3 should satisfy the following (scaled) two-dimensional variational problem of a linearly elastic "membrane" shell (see Thm. 3.4-2; this problem is in fact provisional, since the function spaces and boundary conditions appearing in the definition of the space V(w) definitely need to be modified; see Chaps. 4 and 5, or Sect. 3.5)" r

E V(w)-

{ r / - (r/i)E Hi(w); r / - 0 on 70},

~ aa~'TrT~r(C~~ ~o~ ~n n -

f~ { f : .fi'~ dx3} r l i ~ d y

(,i) e v ( ~ ) , where 1

aa[3~r _

4)~tt aa[3a~r + 2#(aa~aS3r + aar a~), A+2/z

a - det(a~s), and a a~ - a ~. a Is are the contravariant components of the metric tensor of S. Assume next that the space V0(w) contains nonzero functions *7. Then the functions fz, e must be of the form ~

i~.'(~ ") - ~2f~.~(~) fo~ an ~ - ~'~ E n ' , where the functions fi,2 are independent of e (i.e., the exponent p must be set equal to 2 in this case). Furthermore, the leading term

u ~ 9-~ -+ I~3 is independent of the transverse variable x3 and the field r 1 f ~l u~ dx3 satisfies the iollowing (scaled) two-dimensional variational problem o] a linearly elastic "flexural" shell (Thin. 3.4-3)" r e VF(6O):-- { n - (TIi) E Hi(w) x Hi(w) x H2(60); r/i -- Ou?13 -- 0 o n "70, "~a[3(O) -- 0 ill 60},

1 r 3 L aa~vTp'7~'( ) p a / 3 ( r l ) ~ d y - f ~ { f _ : for all n -

]i'2dxa}~Tiv~dY

(ha) E V v ( ~ ) , where

P . , (n) -

0.~ 03 - r2~ O. ~3 - b~ b~, 03 + b~ (0, ~ - r ~ ~. ) + ~ (0o0. - r ~ , ~ )

+ (0o~ + r~~

- r~~),~,

Sect. 3.1]

The three-dimensional equations

141

and the functions Van(r/) and a a ~ r are the same as above. Although the method of formal asymptotic expansions thus admirably serves the purpose of clearly identifying two fundamental classes of possible limit equations, it needs to be substantiated by a convergence analysis. This is why we conclude this chapter by a quick review (Sect. 3.5) of the convergence theorems that will be established in the next three chapters, showing that the scaled unknown u(s) has indeed a limit as --> 0 in an ad hoc functional space, which in each case depends on the geometry of the middle surface S and on the subset V0 of-y. This "refined" analysis also illustrates the limits of the otherwise quite efficient formal approach, as it shows that the "membrane" shells found above need themselves to be subdivided into two subcategories. 3.1.

THE THREE-DIMENSIONAL LINEARLY ELASTIC SHELL

EQUATIONS

OF A

To begin with, we briefly review the main notations, definitions, and results, mostly from three-dimensional linearized elasticity in curvilinear coordinates and from the differential geometry of surfaces, that will be needed in the sequel, and we provide ad hoc cross-references to Chaps. 1 and 2, where these notions have been expounded in detail. Note that the real three-dimensional affine Euclidean space formerly denoted E 3 in Chaps. i and 2 will be henceforth denoted I~3. Greek indices and exponents (except s) belong to the set {1, 2}, Latin indices and exponents (except when otherwise indicated, as when they are used to index sequences) belong to the set {1, 2, 3}, and the summation convention with respect to repeated indices and exponents is systematically used. Symbols such as 6~ or 6~ designate the Kronecker's symbol. The Euclidean scalar product and the exterior product of a, 5 E IR3 are noted 6 . 5 and a A 5; the Euclidean norm of a E IR8 is noted lal. A domain ~ in R n is a bounded, open, connected subset of I~n with a Lipschitz-continuous boundary 0~, the set ~ being locally on one side of 0~. For each integer m > 1, H m ( ~ ) and H ~ ( ~ ) denote the usual Sobolev spaces of real-valued functions. Boldface letters denote vector-valued functions and their associated function spaces. The norm in L2(~) or L2(~) is noted I 9]0,~ and the norm in Hm(f~)

142

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

or ttm(~2), m > 1, is noted II. IIm,~ (s~ct. 1.7). Let w be a domain in I~2 with boundary -),. Let y - (ya) denote a generic point in the set ~ and let 0a := O/Oya. Let 0 E C2(~; I~3) be an injective mapping such that the two vectors

a.(y) := o.o(y) are linearly independent at all points y E -~. These two vectors form the covariant basis of the tangent plane to the surface

s := o(~) at the point 0(y) and the two vectors aS(y) of the tangent plane at 0(y) defined by the relations

form its contravariant basis. Also let

a~(y) A a~(y) a s ( y ) - a3(y):= la~(y)A a2(y)l" Then I~(y)l- z, the vector as(y) is normal to S at the point O(y), and the three vectors ai(y) form the contravariant basis at 0(y); cf. Fig. 2.3-1. Note that (Yl, Y2) constitutes a system of curvilinear coordinates (Sect. 2.1) for describing the surface S. The covariant and contravariant components aaf3 and a afJ of the metric tensor, also called the first fundamental form (Sect. 2.1), the covariant and mixed components ba~ and ~ of the curvature tensor, also called the second fundamental form (Sect. 2.2), and the Christoffel symbols r ~ (Sect. 2.3), of the surface S are then defined by letting (whenever no confusion should arise, we henceforth drop the explicit dependence on the variable y E ~): aao := a a 9af3,

a af3 "= a a 9a f3,

bafj := a 3" O~aa ,

r ~ :=

bfla "- a[3~baa ,

a ~ 9O ~ a ~ .

Note the symmetries: ao, = ~,o,

~~

-- ~ ' ~

bo, -- b,o,

r~, - r~o.

Sect. 3.1]

The three-dimensional equations

143

The area element along S is x/rd dy, where a := det (aa~l). All the functions aa~l, a a~, ba~, bfla,r -a~, and a are thus at least continuous over the set ~. Let V0 denote a dT-measurable subset of the b o u n d a r y 3, of w satisfying

length Vo > O. For each e > 0, we define the sets

a~.- ~• r t "= ~ • {~},

r'

~, ~[,

:= ~ x {-~},

r~ := ~o • [-~, ~].

Let x ~ - (x[) denote a generic point in the set ~ and let 0~ := O/Ox~; hence x a - y a and O~ - Oa. Consider an e l a s t i c s h e l l with m i d d l e s u r f a c e S - 0 ( ~ ) and t h i c k n e s s 2e > O, i.e., an elastic b o d y whose reference configuration consists of all points within a distance 0 is small enough and the data are of an appropriate order with respect to e, the above three-dimensional problems are "asymptotically equivalent" to a "two-dimensional problem posed over the middle surface of the shell". This means that the new unknown should be ~ = ( ~ ), where ~ are the covariant components of the displacement ~ a i " -~ -+ I~3 of the points of the middle surface S - 0(~). In other words, ~ ( y ) a i ( y ) is the displacement of the point O(y) e S; see Fig. 3.1-2.

Sect. 3.2] The three.dimensional equations over a domain independent of e 149

3~ 13t3

Fig. 3.1-2: A two-dimensional shell problem. For e > 0 "small enough" and data of ad hoe orders of magnitude, the three-dimensional shell problem (Fig. 3.1-1) is replaced by a "two-dimensional shell problem". This means that the new unknowns are the three covariant components ~ : ~ --+ IR of the displacement field ~ a i : ~ --+ R 3 of the points of the middle surface S = 0(~). In this process, the "three-dimensional" boundary conditions on F~ are replaced by ad hoe "twodimensional" boundary conditions on 70.

3.2.

THE TttREE-DIMENSIONAI, A D OMAIN INDEPENDENT

EQUATIONS OF

OVER

We describe in this section the basic preliminaries of the asymptotic analysis of a linearly elastic shell, as set forth by SanchezPalencia [1990~ 1992] in the slightly different, b u t in fact equivalent, framework of a "multi-scale" a s y m p t o t i c analysis, t h e n by M i a r a & Sanchez-Palencia [1996], Ciarlet & Lods [1996b, 1996c, 1996d], a n d Ciarlet, Lods & M i a r a [1996]. " A s y m p t o t i c analysis" means t h a t our objective is to study the -+ I~3 as ~ -+ O~ an behavior of the displacement field u~g i'e 9 endeavor t h a t will be achieved by s t u d y i n g the behavior as ~ ~ 0 of the covariant components u i --~ I~ of the displacement field, i.e, the behavior of the u n k n o w n u e = (u~) " - ~ ~ I~3 of the threed i m e n s i o n a l variational p r o b l e m ~ ( ~ e ) described in Sect. 3.1.

150

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

Since these fields are defined on sets ~e that themselves vary with ~ our first task naturally consists in trans]orming the threedimensional problems 7~(~ e) into problems posed over a set that does not depend on e. The underlying principle is thus identical to that followed for plates (Vol. II, Sect. 1.3). As we shall see, there are, however, striking differences! Let

f~ := r0 . - ~ 0 • [ - 1 , 1],

w•

F+ "-- w

1, 1[, •

{1},

r_ .- w • {-1}.

Let x -- (xl, x2, xa) denote a generic point in the set [2 and let (9/ := 0/0xi; hence xa - Ya (a generic point in the set ~ is denoted y - (Yl, y2); cf. Sect. 3.1). With each point x C ~, we associate the point x ~ E ~e through the bijection (Fig. 3.2-1)

7re "X -- (Xl, X2, X3) E ~ ---Y Xe -- (X~) -- (Xl, Lg2, ~g3) E ~ e .

Consequently,

O~ -

Oa and 0~ _ _103.

The coordinate x3 C [-1, 1] will be also called t r a n s v e r s e variable, like x~ E [-e, e] in Sect. 3.1 ("scaled" transverse variable could be preferred; however, no confusion should arise). In order to carry out our asymptotic treatment of the solutions u e = (u~) of problems ~(f~e) by considering e as a small parameter, we must: (i) ~ p ~ i ~ the ~ y th~ ~ k ~ o w ~ ~ = ( ~ ) ~ d m o ~ g e ~ ~ n y th~ ,~to~ ~Id~ ~ = ( ~ ) ~ p p ~ ~ g i~ the fo~m~t~tio~ of p~obt~.~ ~'(~) are mapped into vector fields over the set ~; (ii) control the way the Lamd constants and the applied forces depend on the parameter e. W i t h the unknown u e - (u~) 9~e ~ R3 and the vector fields --+ appearing in the three-dimensional problem 7~(fle), we associate the s c a l e d u n k n o w n u(e) - (ui(e)) 9 -+ ~3

Sect. 3.2]

The three-dimensional equations over a domain independent of e 151

(

0

)

~=~ Z~ I

4

i

I

2

Fig. 3.2-1: Transformation of the shell problem into a scaled problem posed over a set f~ that is independent of e. Each point of the reference configuration of the shell is the image | ") of a point z" = (z~) of the set ~" = ~ • [ - e , e], over which the shell problem is posed in terms of the "natuxal" cuxvilinear coordinates z~. Each point z" = (z~) E ~c is itself the image 7r~z of the point z = (zi) of the set ~ = ~ • [-1, 1] with za = z~ and z"3 = ~zs . Thanks to these changes of variables, the shell problem is transformed into a problem posed over the set 1~.

152

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

and the s c a l e d v e c t o r fields v = (vi) 9~ -+ I~3 defined by the scalings: u~(z e) =: ui(e)(z) and v~(z e) -" vi(z) for all z e - 7fez e ~e.

The three components ui(s) of the scaled unknown u(s) are called the s e a l e d d i s p l a c e m e n t s . We next make the following a s s u m p t i o n s on t h e d a t a , i.e., on the Lamg constants and on the applied body and surface forces: There exist constants A > 0 and/z > 0 independent of e and there exist functions fi E L2(~) and h i C L2(r+ t0 r_) independent of such that A e = A and/~e =/~,

hi, e(z e) = ep+lhi(z)

for all

z e = 7r~zEf~,

for all

z e - re z E F e u r ~

where the exponent p is for the time being left unspecified; needless to say, p is not subjected to the usual rule governing Latin exponents! Since the problem is linear, we assume without loss of generality that the scaled unknown u(e) is "of order 0 with respect to e". This means that the leading term of a formal asymptotic expansion of u(e) is a priori assumed to be of order 0 (Sect. 3.4), an assumption later justified by the proof that the scaled unknown u(s) converges in ad hoc space to a nonzero limit (Chaps. 4, 5, and 6), when the applied forces are of the right orders. A complete justification of the scalings of the unknowns and the assumptions on the data, including the determination of the exponent p, will be given in Sect. 3.4. At this preliminary stage, we simply record three observations: (i) For plates, the "passage from f~ to f~" is identical, but different scalings can be made on the "horizontal" components u a'* and "vertical" components u 3,* of the unknown, and different assumptions can be made on the "horizontal" components fa,~ or h a,6 and "vertical" components f3,e or h 3'~ of the applied forces. This was the basis of the asymptotic analysis set forth for plates by Ciarlet & Destuynder [1979a], also described at length in Vol. II, Sect. 1.3.

Sect. 3.2]

The three-dimensional equations over a domain independent of e 153

(ii) As the problem is linear, there is no loss of generality in choosing ~0 = 1 as the (same) scaling factor for all three covariant components of the displacement field. (iii) For definiteness, we assume that the Lamd constants are independent of s. However, this assumption is merely a special case among a whole class of assumptions, which permit in particular the Lam~ constants to vary with e as s --+ 0 if one so wishes. More precisely, a multiplication of both Lam~ constants by a factor s t, t E IR, is always possible, as we shall explain with more details in the next chapters. The choice t = 0 is merely made here for definiteness. A simple computation then yields the variational problem that the scaled unknown u(s) satisfies over the set ft, thus over a domain that is independent of ~ (as noted in Sect. 3.1 the Christoffel symbols r3'e and FP~e vanish in ~1e for the special class of mappings O considered here; consequently, the functions r3a3(s) and r~3(e ) defined below likewise vanish in ft): T h e o r e m 3.2-1. Let w be a domain in I~2, let 0 E C2(~; I~3) be an injective mapping such that the two vectors aa - OaO are linearly independent at all points of-~, and let so > 0 be as in Thm. 3.1-1. With the functions r i~ , g~ , AiJkl,~ . - ~ -+ R appearing in problem p ( ~ e ) (Sect. 3.1) we associate for each 0 < e < so the "scaled" ]unctions FiP(s), g(e), AiJkl(e) 9-~ --+ I~ defined by

.-

.-

")

g'(,')

for all

ze - ~zE~,

for all

z e - lre z E ~ e ,

for all

z e - ~ezE~.

With any vector field v - (vi) C H l ( f t ) , we associate the s c a l e d l i n e a r i z e d s t r a i n s eillj(s;v ) - ejlli(s; v) E L2(ft) defined by:

.=

1

+

-

) -- _103v3.

p

154

Asymptoticanalysis of linearly elastic shells: Outline

[Ch. 3

Let the assumptions on the data be as above. Then, for each 0 < e 0 in ~,

alIa11 2alla12 \ a 11a11 2allal2 2(a12a12+ a11a22) ) - 2 ~ a ~ 0 in ~, 2 det A - ~-~ > 0 in ~,

where a - det(aa#), we infer from a well-known characterization that the symmetric matrix A(y) is positive definite at all y E ~, and the existence of the constant Ce > 0 follows from the compactness of the set ~; this proves (a). An argument similar to that used in the proof of Thin. 3.3-1 shows that ga~ (e) -- a a~ + O(e) and gi3 (e) - t~i3, where gii(e)(x):= gij'e(xe) for all x e - 7rex e ~ . combined with the definitions (Thm. 3.2-1)

These relations,

imply that

AiJkl(e) -- Aijkl(O) + O(e) and A a ~ a ( e ) - Aa333(e) - 0. For each 0 < e - 2, is a linear combination of u q- 1, U q , U q+l and of their first-order partial derivatives (only the values q = 2 and q - 3 are needed in the sequel). The functions eillJ(S; v) likewise admit formal asymptotic expansions (again resulting from the asymptotic behavior of the functions r,~ (~)) of the form:

le-1 0 (v)+ i (v)+ 2 2 (v)+'", eillJ(e; v ) - - ~ illj(V)+ eillJ seillJ s eillJ where e-1 ~ l ~ ( . ) - 0, e- 1 .ll3(~)-

1 ~o3~,

~(~)-

o~.

I~

~o I[fil( ~ ) _

1 2(0/3va + OqaVfl) -- raflVcr -- ba/3v3' 1

0 e3113(v) -- 0,

3b~l~,~ + 9

,

~ll~(~) - ~ b ; b ~ . . , ~ll~ (v) - o. The asymptotic behavior of the functions g(s) and AiJkt(s) (Thms. 3.3-1 and 3.3-2) also implies that (recall that O E C3(W; I~3) by assumption) g(s) = a + O(e), A i j k t ( s ) V / g ( s ) = AiJk'(O)v/~ + eBijkt, 1 + e2BiJht, 2 + o(s2),

where the functions AiJkl(O) are defined in Thm. 3.3-2.

Asymptotic analysis of linearly elastic shells: Outline

166

[Ch. 3

Note that the above expansions comprise all the terms that will actually appear in an equation at some stage of the subsequent analysis. It does not mean, however, that each one of their specific expressions will be actually needed. As a last preliminary, we also record a simple result frequently used in this volume (as in Vol. II):

T h e o r e m 3.4-1. Let w be a domain in I~2 with boundary 7, let = w • - 1, 1[, and let w E IF(~), p > 1, be a function such that

wO3v d= = 0 for all v E Cr162 Then w

-

-

that satisfy v - 0 on 7 x [ - 1 , 1].

O.

Proof. Let 7~ be an arbitrary function in the space T~(~) and let the function v" ~ -+ R be defined by ~V(zl, z2, t ) d t for all (Zl, z2, z3) E ~2. T h e n v e Ccr

and v = 0 on 3' • [-1, 1]; hence

f n wcp dx - f a wOzv dx = O, and thus w = 0 by a classical property of the space LP(~), p > 1. II The above implication a fortiori holds if fa wO3v dx - 0 for all v E HI(F~) that vanish on r0; this is how it is used in the remainder of this section. We are now in a position to start the cancellation of the factors

of the successive powers of e in the variational equations of problem 7~*(e; ~), until the leading term u ~ of the formal asymptotic expansion can be fully identified. It will be found in this fashion t h a t u ~ satisfies a two-dimensional variational problem, which may be either that of a "membrane" shell or that of a "flexural" shell and that in each case the "right" orders on the components of the applied forces (which we are seeking) appearing in the right-hand sides are simulta-

neously determined. Note that, by contrast with our usual practice, these major conclusions will be formally stated (Thms. 3.4-2 and 3.4-3) only after

Sect. 3.4]

Linearly elastic "membrane" and "flezural" shells

167

they have been established, in a series of eight steps n u m b e r e d (i) to (viii), as this procedure seems more n a t u r a l in the present case. (i) Since the lowest power of e appearing in 7~*(e; fl) is e -2, we are n a t u r a l l y led to first try

1 9 and hi ( e ) _fir,,-2

fi(r

lhi,_ 1

where, here and subsequently, any ]unction fi, r

C

L2(~) and any

]unction h i'r+l E L2(r+ u r_), r > - 2 , is meant to be independent of ~. T h e cancellation of the coefficient of e -2 in the variational equations of p r o b l e m :P* (e; ~) then leads to the equations

ff~ AiJkt(O)e~ltl e -illj l ( v ) v / - a d x - - ff~fi'-2viv/-ddx+ fs t + o r _ hi,-lviv/-adr for all v E V(fl). These equations imply that the ]unctions fi,-2 and h i , -1 cannot be chosen arbitrarily, since we should have in particular

ff fi,-2viv/-a dx + fr+ur_ hi' -lvi ~/-a dr - 0 for all v E V ( f l ) t h a t are independent of x3; to see this, recall t h a t e -1 (v) -- 0, e-1 (v) -- 89 03va, and Consequently,

must let f i , - 2 _ 0 and h i'-1 - O. The expressions of the functions Aijkl(o) and e~-i~l t h e n show t h a t we must have

illJ

-- f~2 (4Aa3Cr3(O)e~[~3e-1 (V) + A3333 _

=

fa

o

03u~O3v~ + ()~ + 2,)03u~

} vZadx - 0

for all v E V ( ~ ) . C o m b i n e d with T h m . 3.4-1, these equations in t u r n imply t h a t

03u ~ - -

0

in f~,

since _ a ~u. 3 %0 - 0 in ~ implies t h a t 03u a0 _ 0 in ~ (the m a t r i x (a af3) is positive definite); hence the leading term u ~ C V ( ~ ) is independent of the transverse variable x3 and it can therefore be identified with

Asymptotic analysis of linearly elastic shells: Outline

168

[Ch. 3

a vector field ~o E Hi(w) satisfying ~o _ 0 on 70. Canceling the coefficient of ~-2 thus yields the relations" r

{~ -

e v(~).-

( ~ ) e a x ( ~ ) ; ~ - 0 on ~o},

e -1 = 0 i n f , . illj (ii) Our second try is thus fi(e) -- I f i ' - I and hi(s) - h i'O. Combined with the relations e -1 - 0 obtained in step (i), the cancelillJ lation of the coefficient of e - t in the variational equations of problem 79"(e; f~) then leads to the equations

fo

AiJkt(O)e~

illJ

+ur_

hi'~

Letting v E V(f~) be independent of xs then implies as in step (i) that the functions fi,-1 and h i'O cannot be chosen arbitrarily, since for such functions v,

for an v ~ v ( ~ ) .

f f fi,-lviv/-ddx-l- fr

+ur_

hi'~

- O.

Consequently, we must let fi,-1 _ 0 and h i'O - 0 and, accordingly, we must then have

faAiJkt(O) ekllt o e-l(v)v/-ddx illJ

= fo 4Aa3~3(O)e~

=0 for aU v E V(f~). Combined with Thm. 3.4-1, these equations in turn imply that e~

-0

and e~l]3 =

aaD ~0

A+2p

Linearly elastic "membrane" and "flezural" shells

Sect. 3.4]

(iii) Our

third try

169

is thus

fi(8 ) __ fi,

O and hi(e) - eh i'l.

The cancellation of the coefficient of s o in the variational equations of problem 79"(~; ft) then leads to the equations (recall that e -1 - 0 ; cf. step (i))" illJ ,A/jkl(0){

o o kll ,llJ(

+

e-~

il,j(")}

+ fo BiJhl'le~ lit e-1illJ (v) d~, = ~ fi'~

fr

+ur_

hi, lviv/-ddr

for all v E V(ft). Observe in passing that the occurrence of the functions e~lll in these equations implies that the formal asymptotic expansion of u(e) should be "at least" of the form u ( e ) - u ~ + ~ u 1 + e2u2 + . . -

.

Let v = r/ E V(w), i.e., v C V(ft) and v is independent of z3. Noting that e illJ - t (v) - 0 for such functions v and using the expressions 0 of the functions AiJkt(O), the relations satisfied by the functions ei[[3 (step (ii)), and the definitions of the functions e~ r and e~ find that

%ll~.eall~(rl)~/~ dx

-

/o 1 /~ = -~

o

aa~O.r 0

0 %ll,eallB(rl)v/-ddx

+UI"_

we

170

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

for all v/E V(w), where the functions

4A~ aC~f3crT .__ ~ a a~

aZ'r + 2p(a a'7 a ~r + a ar a ~(r)

A+2#

are the contravariant components of the s c a l e d t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of t h e shell (already introduced, but without any justification, in Thm. 3.3-2). Let

~,(~)

O"

:= ~(o,~o + oo~,) - r o , ~

- bo,~3

denote the covariant components of the l i n e a r i z e d c h a n g e of m e t ric t e n s o r associated with a displacement field riia' of surface S (Sect. 2.4). Note that Vaf3(v/) E L2(w) if v / - (rIi) E H i ( w ) x H i ( w ) x L2(w). Then remarkably, we precisely have

~o IIf3 - Vaf3(r ) and eallf o 3(r/) - ~'af3(~?) for all ~7 e V(w)

(iv) Define the space

v 0 ( ~ ) := {n e v ( ~ ) ; ~.z(n) - 0 i= ~}, and assume first that

v 0 ( ~ ) = {0}, in which case the shell will be called a linearly elastic "membrane shell. A w o r d of c a u t i o n . This definition is essentially provisional, as it will have to be subsequently amended; cf. Sects. 4.1 and 5.1. The quotation marks emphasize this temporary character, i

Linearly elastic "membrane" and "flezural" shells

Sect. 3.4]

171

Then by step (iii), the vector field ~o should satisfy the following two-dimensional variational problem '~PM(W) ":

r

e v ( ~ ) - {n - ( ~ ) e H~(~); n - o on 70},

fwaa#~rV~r(,~

f pi'~

9

where pz, O :=

for all rl E V(w),

:f2,o dx~ + hi'l( ., 1) + hi't( ., - 1 ) . 1

Besides, the induction stops here since

"~E:~M(W)"is

a bona fide variational problem, which can be studied for its own sake: In this direction, a first observation is that the issue of uniqueness of a solution to problem "7~M(W)'' is immediately resolved when V0(w) - {0}. For, if pi,0 _ 0, we must have in particular

~w aa~ar'y~r(~~176

dy - 0,

and thus 7 ~ ( r 1 7 6 _ 0 in ~o (the scaled two-dimensional elasticity tensor is uniformly positive definite; cf. Thm. 3.3-2 (a)). Therefore, ~0 E V0(w) and thus ~0 _ O. By contrast, the issue of existence of a solution is a delicate one. If Vo -- "Y and the surface S = 0(~) is elliptic, we have already shown through a delicate analysis that problem "~M(W)" has a solution, albeit in the l ~ g ~ space V ~ ( ~ ) - H~(~) • H~ (~ ) • L~(~) (Thins. 2.7-3 and 3.3-2). In the other cases where V0(w) = { 0 } , the c o n c l u s i o n s are even more subtle since the "right" spaces where to seek

a solution turn out to be "abstract" completions (see in particular Thm. 5.6-1)! Such observations already indicate why the definition of a "membrane" shell and that of problem "7)M(W) '' (note the quotation marks) will have both to be modified later. (v) Assume next that the space V0(w) contains nonzero functions, i.e., that

V o ( ~ ) ~ {o}, in which case the shell will be called a linearly elastic "flezural" shell.

172

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

A w o r d of c a u t i o n . Like that of a "membrane" shell, this definition is essentially provisional, as it will have to be subsequently amended; cf. Sect. 6.1. The quotation marks again emphasize this temporary character. II If Vo(w) # {0}, the functions fi, o and h i,1 cannot be chosen arbitrarily since we must have

f pi,~176

+ur_

hi'l~Ti~dF-O

for all r / E ( V o ( w ) - { 0 } ) by definition of problem "~M(W)". Hence we must let fi, o _ 0 and h i' 1 _ 0 and accordingly pursue the induction. Before continuing the induction proper (step (vi)), let us have a second look at the cancellation of the coefficients of e - i and e ~ (steps (ii) and (iii)). Since pi, O _ 0, letting r / - r in the variational equations of problem "7~M(W)'' gives

f a ai3crrTcrr(~0)7a/3 (~0)v/a dy -- O. Hence 7a#(~ ~ - 0 and thus ~o E Vo(w). Since then Call# o - 7a~(~ ~ - 0, the relations e~ 3 - 0 and (A + 2p)e~l13 + Aaa/3e~

-- 0 ill fl

established in step (ii) imply that

0 3 u ~ - e3113 - 0 o

and

e~ll 30 -

cr 0 - 0. ~i ( o ~ ~ + 0 3 ~~) + b~~ 0. - ~i(~162o + o3=~) + b~r

Hence

03u~ -

-

cr 0 (oo( ~ + 2b~i~).

Assume that u i E V(f~). Since each function (0a~ ~ + 2 bcra ~0) is independent of z3, there exists ~i _ (~/1) e V(w) such that

uai _ ~a _ x (Oh ~o + 2baa~o) and u~ - ~J, the first relations forcing in addition the function ~o to be in the space H2(w) and to satisfy the boundary condition 0v~ ~ - 0 on 70

Sect. 3.4]

Linearly elastic "membrane" and "flezural" shells

173

(0v denotes the outer normal derivative along 7) since ~o = 0 on 70 by step (i) (Ex. 1.1 in Vol. II can be handy here). To sum up, we have shown that e~Ij

-- Oinf~,

~O E VF(60)"--

{r/- (~7i) e HI(w) • Hi(w) • H2(w); ~i = 0 ~ 3

Ual __

~al

= 0 011 ")'0, ")'a/3(~'/) = 0 i n w } ,

_ x3 (0a ~g + 2b~ r

and u~ - ~] where r 1 _ (~/1) e V(w).

Since e/~ = 0, the cancellation of the coefficient of e ~ in 7~*(e; ~t) reduces to

ff~ AiJkt(O)e~llt e -illg l(v)v~dx

for all v e V(ft)

-0

By a computation similar to that in step (ii), we then conclude that A a at3etall~ in ft. A+2#

clair3 --0 and elll 3 --

It remains to compute the functions eallt3, 1 as their expressions play a key r61e later. Combining their definitions with the expressions found supra for the components u i1 in terms of ~o and ~ and using the symmetry relations (Thm. 2.5-1) o"

7"

o"

T

we obtain, after some manipulations, 1 1 (0.,11,1 -[- O a U l ) - r ~r ~ 1 - b ~ ~ - -2 ec~ll~--

1 ('"~ l'-'.a

-

+ Oa~)

2

_~{o~o +b~(o~o

Let

_ -

~ 1 1 -- r al~r -- ba~i3

r~ a~ o~r ~

+ ~ 3 { b ~ l ~ 0 + ba" ~b~

o

_ b~a b ~ 3 o o

r ~~~ ) o +

~

174

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

denote the covariant components of the l i n e a r i z e d c h a n g e of curv a t u r e t e n s o r associated with a displacement field yia i of the surface S (Sect. 2.5). Note that

pa~(rl) e L2(w) if r / - (r/i) e HI(u)) • HI(w) • H2(w). Then remarkably, the functions e~ll~ have the following simple expressions in terms of the functions Va~(~ t) (the functions Van(r/) are defined in step (iii) for any r / e V(w)) and pal~(~~ 1

%11~-

7~(r

1

) - ~3p~(r176

9

(vi) We are now in a position to continue the induction V0(w) ~ {0}, with

when

fi(e) = ef i'l and hi(e) = e2h i'2 as our fourth try. The cancellation of the coefficient of s in ~* (e; f~) then shows that (recall that e-tilli = eilli~_ 0; cf. steps (i) and (v))"

fflAijkl(o){ ekllteilli 1 0 (?3) + ekllt 2 e-l(?3))V/-~dx illi illJ + f BiJk"~ lit~-~(.)a~f , i'Xvi ~

dx +

f~+or_ h""2vi v/-d dr

for a U v E V(f~) 9 Let v -- r/ E V(w). Noting that e-t(v) - 0 for illi such functions v and using the expressions of the functions Aiikt(O) and the relations (found in step (v)) satisfied by the functions e illJ' 1 we are led to the equations

fn AiJk~(O)%llteilli ~ o (rl ) v~ dr, 1 [ _a~~o

o

= ~ aa~rT~'(f'l)Va~ (n)V~dy

= f fi,~niV~ddx+fr+ur_ hi,2~Tiv/-ddrforallrleV(w).

Sect. 3.4]

Linearly elastic "membrane" and "flezural" shells

175

Hence the functions fi, t and h i'2 cannot be chosen arbitrarily, since we must have

fwfi'lrliV/-ddy + f r

+ur_

hi'2rli~dr - O

for all r/ E ( V 0 ( w ) - {0)); consequently, we must let fi,1 _ 0 and h i'2 - O. But then, letting r / - ~t in the above variational problem shows that

Hence 7a~ (~ t) = 0 and consequently,

c v0@), since on the other hand, ~l e V(w) by step (v). (vii) As a preparation to step (viii), let us further exploit the cancellation of the coefficient of e in 7~*(~; 12) when V0(w) # {0}, which now leads to the equations

fftAiJkl(O){ ek[[leillj(v) 1 0 + e~llle-l(v))v/-adx i[IJ -4- f~ BiJkt'ie~lll e-1 illj(V)dx - 0 for all v C g(f~), since we are now assuming that fi, x = 0 and h i'2 --O. Given an arbitrary element ~/ in the space Vy(w) defined in step (v), let v(~/)= (vi(~l)) be defined by va(r/) := zsI2b~,r/~ + 0at/s} and v3(r/):= 0. Since v(r/) e V(i2), we may let v = v(r/) in the above equations; this leads to the equations:

ft AiJkl(O) ekllteillj 0 (v(r/))~dx +4

/a

/o

+

r

l oa ~13) v/-d dz

176

[Ch. 3

Asymptotic analysis of linearly elastic shells: Outline

Remark. The relations -),a~(rl) = 0 in w satisfied by the functions rl E VF(w) are not needed at this stage; in other words, the above equations are in fact valid for all rl - (r/i) e Hi(w) • Hi(w) • H2(w) that satisfy the boundary conditions r/i = Ourl3 = 0 on 70. i (viii) We conclude the induction when V0(w) r {0}, with

fi(e) __ e2 fi, 2 a n d hi(e) - ~3hi'3 as our fifth, and final, try. The cancellation of the coefficient of e 2 in :P*(e; 12) then shows that (recall that e-lilli - eillJ~_ 0)" fa

3

-1 (v)}v/-~ d x

+ foBiim, l~l ehllleillj 1 o (v)+ ekllZ 2 e-1 ill./(v)} dx

...Bijkl,2elklit illJ(v) dx - f "f"2viv/-ddx+ e -1

+ur_

" h"3v~v/Sdr

for all v C V ( ~ ) . Observe in passing that the occurrence of the functions e3]lz in these equations implies that the formal asymptotic expansion of u(e) be "at least" of the form U(e) -- U 0 -~- eU 1 -~ e2U 2 -~- e3U 3 -~- e4U 4 ~ - ' ' " ,

as e~llt is a function of u 2 u 3 and u 4 Let v = rl E VF(w). Then for such functions v, ~

e-l(v)

illJ

0

:

-

0,

9

= 0

1

=

+

a

so that we are left with the equations

faA~jh~(0) ekllteill 1 1 I ( rl ) v/adx + 4 in Aanaa(O)e21jn{bTarl~ + ~Oay3}v/adx 1 -+-4 .fc~ Ba3a3' 1 e~li3 1 {brarlr + -~Oarl3 1 }~

=

fp~'2mv~dy d~

dx

for all rl E VF(w),

0 (v)-0

Sect. 3.4]

Linearly elastic "membrane" and "flezural" shells

177

where p,,29 := f ~

1

It," 2 dx3 -4- h "s (. ,

1) + h""s (., - 1 ) .

Subtracting the equations found in step (vii) from these equations, we find that

f~ AiJkl (O)e~lll{eillj(~l) t O ( v ( ~ l ) ) } ~ d x _ ~ p"" 271iV/-~dy - eillJ for all v/e VF(w). First, the relations (established in step (v)) t -0and eall3

t A aaf3"l inf~ e3113 = - A + 2------~ ~all~ '

and the relations esllst(~/) _ esll 3o (v(r/)) - 0 together imply that

AiJk'(O)e~llt{e~llJ(~l) - ei~ _

_

AOt~a'v[Nh,~l

- "-"

el

0

0. For each ~ > 0, the shells are subjected to applied body and surface forces. For each e > 0, let ui(e) denote as in Sect. 3.2 the three scaled displacements, i.e.~ the scaled covariant components of the displacement field of the points of the shell; each scaled displacement ui(e) is thus defined over the fixed domain f~ = w • 1, 1[. Assume first that 70 = 7 and that the surface S is elliptic, in the sense that its Gaussian curvature is > 0 everywhere. Then Ciarlet & Lods [1996b] have shown that, if the applied body force density is O(1) and the applied surface force density is O(e) with respect to 6 in the sense of Tam. 3.4-2, the scaled unknown u(e) = (ui(e)) converges in Hl(f~) • Hl(f~) • L2(f~) as ~ --+ 0 to a limit u, which is independent of the transverse variable (this convergence result has been recently improved by Mardare [199Sa], who obtained art O(~ 1/6) error estimate). Furthermore, the average ~ := 89f~l u dx3 satisfies the s e a l e d t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m 7~M(W) of a l i n e a r l y elastic elliptic m e m b r a n e shell:

r e





f aaf3~r 7at (~) 7af3 (r/) V/-ddy

= ~pi'~

for all rl - (rli) C VM(w),

where the functions a afl~r, ")'aft(r/), and pi, O are defined as in Thin. 3.4-2. Notice, however, that the space VM(W) does not coincide with the space V(w) found in Thin. 3.4-2! The detailed proof of this convergence result, which occupies most of Chap. 4, is concluded with Thin. 4.4-1. Naturally, these equations have to be "de-scaled'~ so as to be expressed in terms of "physical" unknowns and data. To this end, we let ~e(y) = ~(y) for y E ~ (in view of the scalings ue(x `) = u(e)(x) for x e - rex C f~); it is found in this fashion that the de-scaled

Summary of the convergencetheorems

Sect. 3.5]

185

unknown ~e satisfies the two-dimensional variational problem:

Ce E VM(W),

L aa~~176 = f p~'~wV~dy fo~ an ,1 = (w) Jw

VM(W),

where 4)~ePe aa~a~r + 2pe(aa~a~r + a a r a ~ ) , ,Xe + 2# e o

/

~

~

9

~

o

f',~ d ~ + h ; ~ + h ',~ ~na h~ ~ : : h ',~(.

+~)

e

Note that these equations are of the form announced in Sect. 2.7. As shown by Ciarlet & Lods [1996a] and Ciarlet & SanchezPalencia [1996] (under rather stringent regularity assumptions, later substantially relaxed by Lods & Mardare [1998a]; cf. Thm. 2.7-2), the conjunction of the two assumptions "V0 - V" and "S is elliptic" provides a first instance where the space VF(W) "-- {r/--(r/i) e Hi(w) • HI(w) • H2(w); ~?i - 0v~73 - 0 on 70, 7a~(~/) = 0 in ~} contains only the function r / = 0. The space VF(W) was introduced by Sanchez-Palencia [1989a]. Then Ciarlet and Lods [1996d] studied all the "remaining" cases where VF(w) = {0}, for instance, when the surface S is elliptic but 0 < length 70 < length V (as shown by Vekua [1962] and Lods & Mardare [1998a]), or when S is a portion of a hyperboloid of revolution and V0 is "large enough" (as shown by Sanchez-Palencia [1993] and Mardare [1998c]), etc. To give a flavor of their results, consider the most common case, where the space Vo(c,,) := {n ~ Hi(,,,); ,7 - o on 7o, ~',l~(n) = 0 in ~,},

186

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

which contains VF(w), "already" reduces to {0}, or equivalently, when the semi-norm

l" [M'~--(~i)~ -+

1271M"- { ~ lT,~(n)i~),,,,}

1/2

a,/3

becomes a norm over the space := { n e

n - 0 on 70).

In this case, if the applied forces are "admissible" in a specific sense (too technical to be reproduced here; cf. Sect. 5.5), the average !2 fl_ 1 u ( e ) d x 3 converges as e -4 0 in the space

V~M(W) '-- completion of V(w) with respect to I" IM. A convergence result also holds for the scaled unknown u(e) itself (again too technical to be reproduced here). Furthermore, the limit satisfies the scaled t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m 79~M(W) of a l i n e a r l y elastic g e n e r a l i z e d m e m b r a n e shell:

r e V~M(~O)and B~M(r O) -- L~M(n) for all r/E

V~M(w),

where B~M is the unique extension to V~M(W) of the bilinear form (r

already found in the variational equations of an elliptic membrane shell (see supra) and L~M 9V~M(W) -4 IR is an ad hoc linear form, determined by the behavior as e -4 0 of the admissible forces. Notice that the space V~M(W) neither coincides with the space V(w) found in Thm. 3.4-2! The detailed proof of this convergence result, which occupies most of Chap. 5, is concluded with Thm. 5.6-1. A particularly noteworthy feature of such variational problems is that they provide instances of "sensitive problems", introduced and studied by Lions & Sanchez-Palencia [1994, 1996, 1997].

Summary of the convergence theorems

Sect. 3.5]

187

Remark. In the "last", but seemingly uncommon, case where VF(w) -- {0} but I 9IM is a "genuine" semi-norm over the space V(w), a similar convergence result can be established, but instead in the completion ~r~M(W) with respect to I" IM of the quotient space .

-

The limit found in this fashion in the space ~r~M(W) then satisfies the scaled two-dimensional variational problem of a linearly elastic generalized membrane shell "of the second kind"; see Thm. 5.6-2. II Finally, Ciarlet, Lods & Miara [1996] have considered the case where the space VF(w) contains non-zero functions. This assumption is satisfied in particular if S is a portion of a cylinder and 0(70) is contained in one or two generatrices of S (as shown by Lods & Mardare [1998a]; see also Ex. 3.4) or if S is contained in a plane, i.e., the shell is a plate. They then showed that, if the applied body force density is O(e 2) and the applied surface force density is O(e 3) with respect to e in the sense of Thm. 3.4-3, the scaled unknown u(e) = (ui(e)) converges in Hi(12) to a limit u, which is independent of the transverse variable. Furthermore, the average ~ "- 1 f ! l u din3 satisfies the s c a l e d twod i m e n s i o n a l v a r i a t i o n a l p r o b l e m T'F(w) of a l i n e a r l y elastic f l e x u r a l shell: r E V f ( w ) : = {r/--(r/i) E Hi(w) • HI(w) x H2(w); 7/i - 0v7/3 - 0 on 3'0,7a#(r/) - 0 in w},

1Z for all r / = (r/i) E VF(w),

where the functions a a#~rr, pa#(r/), and pi, 2 a r e defined as in Thm. 3.4-3. Notice that, for once, the "right" space Vv(w) was already found in this theorem! The detailed proof of this convergence result is the object of Thin. 6.2-1. In order to acquire physical significance, these equations must be de-scaled, like those of a membrane shell. The de-scaling then shows that the de-scaled unknown ~e satisfies the two-dimensional

188

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

variational problem:

r ~ vp(~), C3 f aaf~ar, e

Y J~

P

par(~e)pa#(17)~/-a dy - J~ Pi'e~Ti~/a dy for all r / = (~/i) e VF(W),

where

~~,~

._.- 4 ~ , ~ ~ ~

+ 2,~(~~ ~ + ~~'~),

Ae + 2# e 9

f ~

9

o

.

.

;',~ : : j _ I ',~ d ~ + h ; ~ + h ''~_ ~ a h~ ~ : : h ',~(., +~). $

Note that these equations are of the form announced in Sect. 2.6.

All these convergence results heavily rely on the inequalities of Korn's type on a surface established in Chap. 2, first for a general surface (Thm. 2.6-4), then for an elliptic surface (Thm. 2.7-3). Not only do these inequalities play a crucial r61e for establishing the existence and uniqueness of the solution to the "limit" two-dimensional equations (as already shown in Sects. 2.6 and 2.7), but they also constitute the basis for proving "three-dimensional" inequalities of Korn's type, either for a family of general shells or for a family of elliptic membrane shells, that are themselves the keystones of the convergence proofs. These convergences for the displacements have been recently complemented by Collard & Miara [1999] who have established the convergence of the corresponding linearized stresses, by Giroud [1998] who has considered linearly elastic shells made of nonhomogeneous and anisotropic materials, and by Xiao Li-ming [1998, 1999a] who has considered time-dependent linearly elastic membrane and flexural shells. Ciarlet & Lods [1996c, 1996d] have also fully justified the twodimensional Koiter equations for a linearly elastic shell, described at the beginning of Sect. 2.6, by combining the above convergences with

Sect. 3.5]

Summary of the convergence theorems

189

former asymptotic analyses of Koiter's equations due to Destuynder [1985] and Sanchez-Palencia [1989a, 1989b]. More specifically, Ciarlet Lods [1996c, 1996d] have shown that the average 1 fe_e ue dx~ and the solution ~ g of Koiter's equation have for each kind of shell the same asymptotic behavior as ~ -~ O.

The detailed proof of this result is the object of Thms. 7.2-1 to 7.2-3. A somewhat unexpected phenomenon, identified by Ciarlet [1992a, 1992b], arises when "a shell becomes a plate": Suppose first that the middle surface S "converges" in a natural sense to a planar domain, while the thickness 2~ is held fixed: Then the solution of the three-dimensional shell equations converges toward that of the threedimensional plate equations (Ex. 3.5). If then e approaches zero, the solution of the three-dimensional plate equations converges toward the solution of the two-dimensional plate equations, i.e., those of the linear Kirchhoff-Love theory, which simultaneously incorporate membrane and flexural terms (Vol. II, Thm. 1.4-1), regardless of the geometry of S and of the boundary conditions. By contrast, suppose first that e approaches zero while the middle surface is held fixed. Then the above ~onvergence theorems show that the three-dimensional solutions converges towards a two-dimensional limit that satisfies either the elliptic membrane, or the generalized membrane, or the flexural equations, according to the geometry of S and to the boundary conditions. If then the surface S becomes planar, the limit equations obtained in this process are thus either the membrane, or the flexural, plate equations. In other words, "the two passages to the limits do not commute"! Additional considerations about this puzzling question are found in Sanchez-Palencia [1994] and

Loa [1996]. As shown by Busse, Ciarlet & Miara [1997], the two-dimensional equations of a linearly elastic "shallow" shell in curvilinear coordinates (these equations are given in Sect. 7.6) can be also justified by means of a convergence theorem, which is reminiscent of that used for a linearly elastic shallow shell in Cartesian coordinates (Vol. II, Chap. 3). We recall that, according to the definition justified by Ciarlet & Paumier [1986] in the nonlinear case and by Ciarlet & Miara [1992a] in the linear case, a shell is "shallow" if, in its reference configuration, the deviation of its middle surface from a plane is of the order of its thickness (see again Vol. II, Chap. 3 for details).

190

Asymptotic analysis of linearly elastic shells: Outline

[Ch. 3

EXERCISES

3.1. Let the assumptions be as in Thin. 3.3-2. (1) Show that the uniform positive definiteness of the two-dimensional elasticity tensor on S can be also established in a manner reminiscent of that used in Thm. 1.8-1 for establishing the uniform positive definiteness of the three-dimensional elasticity tensor. (2) Show that yet another proof consists in adapting that suggested in Ex. 1.8 in the three-dimensional case. 3.2. Let a a ~ r denote the contravariant components of the twodimensional elasticity tensor of a shell (Thm. 3.3-2), and let # > 0 be given. Show that there exists a constant A0(/z) < 0 such that, if X > )~0(#), there exists a constant c > 0 such that E

Iraqi2 -< caa/3~r(y)tarta[3

a,/3

for all y C ~ and all symmetric matrices (tat3). Remark. Such a uniform positive definiteness of the two-dimensional elasticity tensor is established in Thm. 3.3-2 under the assumptions )~ >_ 0 and # > 0. 3.3. Consider a linearly elastic shell whose middle surface is a portion S - 0(~) of a sphere, with (Fig. 2.1-3) := {(~, , ) ~ R 2 ; o < u 2 + v 2 < r2},

( O(u, v) :=

2R2u 2R2v u 2 + v 2 - R 2) u 2 + v ~ + R 2' u~ + v 2 + R 2' Ru2 ~- v 2 + R 2 '

i.e., stereographic coordinates are used for representing the surface S. This spherical shell is subjected to a boundary condition of place along its entire lateral face, i.e., 7o = 7. (1) Show that such a shell is a "membrane" shell, according to the definition given in Thm. 3.4-2. Hint: Use Ex. 2.13. (2) Compute explicitly the functions a a/3~r, 7at3(r/), and a appearing in the formulation of the associated variational problem "79M(W)'' (Thm. 3.4-2).

Ezercise8

191

(3) Carry out the same computations when the surface S is represented by means of spherical coordinates (Fig. 2.1-3). Remark. The expressions sought in (2) and (3) immediately follow from Ex. 2.1 (2). 3.4. Consider a linearly elastic shell whose middle surface is a portion S - 0(~) of a circular cylinder, with (Fig. 2.1-2)

:= (R cos

R sin

z).

This cylindrical shell is subjected to a boundary condition of place along both "vertical" portions of its lateral face, i.e., 70 - {(0, z) C I~2; 0 _< z _ h} U {(Tr, z) E I~2; 0 _ z _< h}. (1) Show that such a shell is a "flexural" shell, according to the definition given in Thm. 3.4-3. (2) Compute explicitly the functions a a ~ r , 7a~(r/), pa~(~/), and a appearing in the formulation of the associated variational problem T'F(w) (Thm. 3.4-3). Remark. The sought expressions follow from Ex. 2.1 (1). (3) Assume now that this shell is subjected to a boundary condition of place along its entire lateral face, i.e., that V0 - V. Is it still a "flexural" shell? 3.5. Let there be given an injective mapping 0 = (~i) E C2(~; I~3) such that the two vectors 0a0 are linearly independent at all points of ~. Following Ciarlet [1992a], consider a one-parameter family of mappings O(t) - (Oi(t)) 9 w ~ I~3 defined for 0 ~ t ~ 1 and (yl, y2) E ~ by e

(t)(yl, y2) : te (y , y2) + (1 - t)y ,

~3(t)(Yl, Y2) -- t~3(Yl, Y2), and assume for simplicity that the contravariant components of the applied forces are independent of t. Let u~(t) E V ( ~ e) denote for 0 < t ~ 1 the solutions of the corresponding variational problems ~(~2~), as described in Sect. 3.1 but now parametrized by t.

192

Asymptoticanalysis of linearly elastic shells: Outline

[Ch. 3

Show that the mapping t E [0, 1] -+ ue(t) E V(I2 e) is continuous. In particular, ue(t) --+ ue(O) in Hl(f~ e) when t -+ 0 +, i.e., when "the shell becomes a plate", where ue(O) E V(f~ e) satisfies the threedimensional equations of a clamped plate:

ffl BiJkt, eei~(ue(O))e~t(ve)dxe- ffl fi'e edxe+ f 9

~ u r ~_

hi'e iecIF

where

Hint: Observing that the Lax-Milgram lemma can be proved by means of the contraction mapping theorem (Lions & Stampacchia [1967]), use the local uniform ellipticity of the associated bilinear forms to show that the contractions are also loeaUy uniformly contraeting.

CHAPTER 4 LINEARLY SHELLS

ELASTIC

ELLIPTIC

MEMBRANE

INTRODUCTION

A linearly elastic elliptic membrane shell is one whose middle surface S = 8(~) is elliptic, i.e., that has a Gaussian curvature that is everywhere > 0, and which is subjected to a boundary condition of place along its entire lateral face (Sect. 4.1). The infinitesimal rigid displacement lemma on an elliptic surface (Thm. 2.7-2) thus shows that an elliptic membrane shell provides one instance where the space VF(6Q) -- {17 --(~7i) e Hl(ag) x H i ( w ) x H2(Qg); i T i - 0v~73 - - 0 oil ")'0, =

0

reduces to {0}. The other instances where Vy(w) = {0} are provided by the "generalized membrane" shells, which will be studied in the next chapter. As we shall see, whether VF(w) = {0} or VF(W) r {0} is the fundamental criterion for classifying linearly elastic shells: Those corresponding to VF(w) = {0} constitute the membrane shells, while those corresponding to Vv(w) # {0} constitute the flezural shells (Chap. 6). The purpose of this chapter is to identify and to mathematically justify the two-dimensional equations of a linearly elastic elliptic membrane shell, by establishing the convergence in ad hoc functional spaces of the three-dimensional displacements as the thickness of such a shell approaches zero. More specifically, consider a family of linearly elastic elliptic membrane shells with thickness 26 approaching zero and with each having the same middle surface S = 8(~). As in Chap. 3, the associated three-dimensional problems, posed in curvilinear coordinates over the sets Fte = w• - e, s[, are transformed for each e > 0 into equivalent problems, but now posed over the set ~ = w • 1~1[, which

194

Linearly elastic elliptic membrane shells

[Ch. 4

is independent of e. This transformation relies in a crucial way on appropriate scalings of the unknowns u~ (the covariant components of the displacement field) and assumptions on the Lam6 constants

)i ~ and Ize and on the contravariant components fi, e of the applied body forces (for simplicity, we assume in this introduction that there are no applied surface forces). More specifically, we define the scaled unknown u(e) = (ui(e)) by letting u~(x e) - ui(e)(x) for all x ~ - ~r~x e ~e, where 71"e(Xl, X2, X3) (Xl, X2, EX3). Guided by the formal asymptotic analysis of Sect. 3.4, we then assume that there exist constants ,k > 0 and # > 0 and functions fi E L2(f~) independent of e such that -

-

%e=)~

and

#e=#,

fi,~(x ~) - f i ( z ) for all x ~ - ~'ex E ~26. It is found in this fashion that the scaled unknown u(e) satisfies a variational problem of the form (Thin. 4.1-1):

u(e) -- (ui(~)) E V(f~) -- {v -- (vi) E Hl(f~); v - 0 on "y • f n AiJkl(e)eklll(e; u(e))eillj(e; v ) ~ ) =

[--I,1]},

d~,

fo

for all v e V(f~),

where, for any vector field v = (vi) E Hl(f~), the scaled linearized strains eillj(e; v) -- ejlli(e; v ) E L2(12) are defined by"

~jl~(~; ~) - ~I ( o ~ + o ~ ) ~ll~ (s;

")

1(i

= ~ ~ o3,~ + o ~ 3

)

r P~

(e)vp ,

- r~3 (e)~,

eall3(e; v) = e103v 3. To begin with, we establish several properties of "averages with respect to the transverse variable" that will be of frequent use (Thm. 4.2-1). T h e n we prove a crucial three-dimensional inequality of Korn's type (Thin. 4.3-1): Given a family of linearly elastic elliptic membrane shells with each having the same (elliptic) middle surface S -- 0(~),

Introduction

195

there exists a constant C such that, for e small enough and for all = (~) E v(~),

0 strongly converges in the space Ht(fl) • Ht(f~) x L2(~t) as r -+ 0 and that u = lime_,0 u(e) is obtained by solving a two-dimensional problem. More specifically, we show that the limit u is independent of the transverse variable and that ~ - ~1 f_l 1 u dx3 satisfies the following (scaled) two-dimensional variational problem of a linearly elastic membrane shell:

r -(r

e v M ( ~ ) - H ] ( ~ ) • H0~(~) • L~(~),

1

O"

~ o , ( ~ ) - ~ ( 0 , , ~ + oo~,) - r o , , ~ - bo,,~, aa~ r _

4)~p aa~ a,Tr + 2#(aa(r a~r + aar a~,r) ' )~+2#

the functions 7a~(r/) and a a~ar being respectively the covariant components of the linearized change of metric tensor associated with a , displacement field yia ~ of the middle surface S (Sect. 2.4) and the contravariant components of the (scaled) two-dimensional elasticity tensor of the shell. To conclude this chapter, we review the existence, uniqueness, and regularity properties of the solution to the above variational problem and we describe the associated minimization problem and boundary value problem (Thm. 4.5-1). We also rewrite these two-dimensional equations and the fundamental convergence theorem in terms of descaled unknowns and data, thus providing a justification in terms of

196

Linearly elastic elliptic membrane shells

[Ch. 4

"physical" quantities of the two-dimensional equations of a linearly elastic membrane shell (Thins. 4.5-2 and 4.6-1). In particular, the limit displacement field ~ a i of the middle surface is such that ~e _ (i~) satisfies the following minimization problem: ~e C VM(W) and j ~ ( ~ e ) = inf j ~ ( r / ) , r/eVM(tO)

where the two-dimensional energy j ~ " V M ( w ) ~ I~ is defined by

J ~ ( Y ) = -~

e a a~ 'Tr' eVar ( Y ) Va~ ( Y ) v/-a d y _

L{f_

}

fi, edxe3 ~Tiv/-ddy, e

and a a[J(rT, e =

Ae

4.1.

+ 2# e

aal3 aO'r + 2/.te (a a~

+ a ar a13O').

LINEARLY ELASTIC ELLIPTIC MEMBRANE SHELLS: D E F I N I T I O N , E X A M P L E , A N D A S S U M P T I O N S O N T H E DATA; T H E THREE-DIMENSIONAL EQUATIONS OVER A D O M A I N I N D E P E N D E N T OF g

Let w be a domain in ]~2 with boundary 7 and let 0 C C2(~; I~3) be an injective mapping such that the two vectors OaS(y) are linearly independent at all points y C ~. A linearly elastic shell with middle surface S = 8(~) is called a l i n e a r l y e l a s t i c elliptic m e m b r a n e shell if the following two conditions are simultaneously satisfied (the definitions and notations are those of Sect. 3.1): (i) The shell is subjected to a (homogeneous) b o u n d a r y cond i t i o n of place along its entire lateral face 0 ( 7 • I - e , e]), i.e., the displacement field vanishes there; equivalently, 70 -- "Y.

(ii) The middle sur]ace S is elliptic, in the sense that there exists a constant c such that

i~12 ~ alba~(y)~a~[ c~

for a11 y E ~ and a11 (~a) E R 2

Sect. 4.1]

Definition, ezample, and assumptions on the data

197

Fig. 4.1-1: A linearly elastic elliptic membrane shell. A linearly elastic shell whose middle surface S = 8(~) is a portion of an ellipsoid E, and which is subjected to a boundary condition of place (i.e., of vanishing displacement field) along its entire lateral face 19(7 • [-e, e]) (darkened on the figure), provides an instance of an elliptic membrane shell. Note that stereographic coordinates (Fig. 2.1-3) afford the representation of such a surface S. Elliptic membrane shells provide a first instance (70 = 7 and S is elliptic) where the space VF(w) = {~ = ('7,) e Hi(W) • Hi(oJ) • H2(oJ); ~, = 0~Os = 0 on 70, 7o~C,7) = 0 in

~},

which is the key to the classification of linearly elastic shells, reduces to {0} (in fact, a larger space "already" reduces to {0} in this case; cf. Tlun. 2.7-2). The "generalized membrane shells" (Chap. 5) exhaust all the remaining cases where V~(~) = {0}.

where the functions ba~ : ~ --~ I~ are the covariant c o m p o n e n t s of the c u r v a t u r e tensor of S (this definition was a l r e a d y given in Sect. 2.7). This a s s u m p t i o n m e a n s t h a t the Gaussian curvature of S is everywhere > 0; equivalently, the two principal radii of curvature are either both > 0 at all points of S, or both < 0 at all points of S (see Sect. 2.2 for a detailed exposition of these notions). A shell s u b j e c t e d to a b o u n d a r y c o n d i t i o n of place along its entire lateral face a n d whose middle surface is a p o r t i o n of an ellipsoid provides a n e x a m p l e of a linearly elastic m e m b r a n e shell (Fig. 4.1-1).

Let there be given a linearly elastic elliptic membrane shell such that 8 C C2'1(~; IR3). T h e n the following inequality of K o r n ' s t y p e on the elliptic surface S = 8 ( ~ ) holds ( T a m . 2.7-3): There exists a

Linearly elastic elliptic membrane shells

198 c o n s t a n t CM

[Ch. 4

such that

11,7~11~~,~

~ ,~3,o,~

_< CM

~

I~,~(.11o2, ,,,

fo~ ~11. = (vi) e v M ( ~ ) : = H~(~) • H~(~) • L2(~), where the functions 1

7 ~ ( n ) := ~ ( 0 ~ , + 0 ~ )

O"

- r~.

- ba/3r/3

are the covariant components of the linearized change of metric tensor associated with a displacement field ~ia 2 of the surface S; the subscript "M" announces that VM(W) is the functional space over which the limit two-dimensional equations of such a membrane shell are posed (Thin. 4.4-1). This inequality, consequence of the definition of an elliptic membrane shell, will be the key to the ensuing analysis of this chapter. A w o r d of c a u t i o n . The definition of a linearly elastic elliptic membrane shell thus depends only on the subset of the lateral ]ace where the shell is subjected to a boundary condition of place (this subset should be the entire lateral face) and on the "geometry" of its middle surface (its Gaussian curvature should be > 0 everywhere). This definition is thus independent of the particular system of curvilinear coordinates employed for representing the surface S. m If assumptions (i) and (ii) are satisfied and O e C2'1(~; IR3), we thus have

{ . - ( y i ) e H~(w) • H~(w) x L2(w); 7 a ~ ( . ) -

0 in w} - {0}.

Hence linearly elastic elliptic membrane shells provide a first instance (70 = 7 and S is elliptic) where the space (already introduced in Thin. 3.4-3)

VF(~) "-- {n = (~) e HI(~) • H~(~) • H2(~); ~?i = Ou~3 = 0 on 70, 7a~3(~) = 0 in w} a fortiori reduces to {0) (we recaU that Ov denotes the outer normal derivative operator along 7; the subscript "F" reminds that this space is central to the study of flezural shells, undertaken in Chap. 6).

Definition, ezample, and assumptions on ~he da~a

Sect. 4.1]

199

The importance of this observation lies in that the issue of whether VF(w) = {0) or VF(w) ~ {O) is the basis of the classification of linearly elastic shells: A shell is caUed a l i n e a r l y e l a s t i c m e m b r a n e shell if VF(w) = {0) or a l i n e a r l y e l a s t i c f l e x u r a l shell if VF(~)

# {0).

In this direction, note that elliptic membrane shells far from exhaust all the instances where VF(w) = {0), the remaining instances corresponding to the generalized membrane shells studied in the next chapter. The formal analysis of Sect. 3.4 then naturally leads us to make the following s e a l i n g s of t h e u n k n o w n s and a s s u m p t i o n s o n t h e d a t a for a family of linearly elastic elliptic membrane shells with each having the same (elliptic) middle surface S = 0(~) as their thickness 2~ approaches zero. First, we define the s c a l e d u n k n o w n u ( e ) - (ui(e)) by letting

u~(x ~) "-- ui(6)(x) for all x e - 7r~x e ~ .

Next, we require that the Lamd constants and the applied body and surface force densities be such that

)~ - )~ fi,~(x e) - f i ( x )

h',~(~ ~) - ~h'(~)

and for all

#e _ #, x ~ = 7r~x e a ~,

fo~ ~11 ~ - ~

e r ~W u r ~- '

where the constants )~ > 0 and ~ > 0 and the functions f i E L2(f~) and h i E L2(r+ u r_) are independent of e (Fig. 3.2-1 recapitulates the definitions of the sets ~e, f~, r ~ , r + , r ~_, a n d r _ ) . Remark. For notational brevity, the functions f i and h i stand for the functions that were respectively denoted fi, 0 and h i' 1 in Sect. 3.4. II As an immediate corollary to Thm. 3.2-1 (simply corresponding to p -- 0), we obtain the problems satisfied by the scaled unknown over the set fl, thus over a domain that is independent of ~:

200

Linearly elastic elliptic m e m b r a n e shells

[Ch. 4

T h e o r e m 4.1-1. Let w be a domain in I~2, let 0 E C2(~;IR 3) be an injective mapping such that the two vectors a a - - OaO are linearly independent at all points of-~, and let eo > 0 be as in Thm. 3.1-1. Consider a family of linearly elastic elliptic membrane shells with thickness 2e with each having the same elliptic middle surface S - 0(~). Let the assumptions on the data be as above. Then, for each 0 < e 0. If no particular assumption is made on the geometry of the surface S, it will be shown in the next chapter (Thm. 5.3-1) that there exist constants el > 0 and C > 0 such that, for all 0 < e < ez and all fields v - (v~) E H1(12) vanishing on the set 3'0 • [-1, 1], 1/2

. Ilvili *

C

2

-
0 satisfies. The following result is due to Ciarlet & Lods [1996b, Thm. 4.1]. T h e o r e m 4.3-1. Assume that 0 E C3(~; I~3) and let eo > 0 be defined as in Thm. 3.1-1. Consider a family of linearly elastic elliptic membrane shells with thickness 2e with each having the same elliptic middle surface S = 0(-~). Define the space

V ( ~ ) " - {v - (vi) e H I ( ~ ) ; v - 0 on 7 • [-1, 1]}.

Then there exist a constant el satisfying 0 < ex (V, 01 v, ~2 v, O3t;) E H - I ( G ) is an isomorphism.

Sin~ o3~(~) = 2~(~,13(~) + r~3(~)~.(~)) - ~o~3(~), w. n~.t have, for all 7~ E ~9(ft),

and consequently, there exists by (i) a constant cl independent of e such that

whe~ ll" I1-~,. denotes th~ norm in H-~(a). Hen~ 0s~o(~) -~ 0 in H-~(a). We next have the identity

- ~ o (~ts~(~) + ~r~(~)~.(~)) imply that

Sect. 4.4]

Convergence of the sealed displacements as e ~ 0

219

since OaOoua = 0 in ~'(12). Denoting by < . , 9> the duality between 7)'(12) and T)(12), we thus have, for all qo e T)(12),

< o, (~o,l~(~) + ~r~(~)~.(~)), ~ >

= -~ f. {~ol,~(~) + r~(~)~.(~)} 0,~ a~, and consequently, there exists c2 independent of e such that

II0, (~,i~(~) + ~r~(~)~(~))II-x,n ~ ~ , by (i). The last term in the expression of O~Osua(e) is treated analogously. Hence O~Osua(e) -+ 0 in H-l(12). Finally, we have, for all ~o E :D(12),

< 0303ua(e), ~o

>=- fn 03ua(e)Os~odz

_- _2e fm {e~llS(e) + r:s(e)u~(e)} Os~odm+ e2 fa e3113(e)Oa~dx,, and consequently, there exists by (i) a constant ca independent of e such that ll0303u~(e)ll-x,n

< cse,

Hence 0303ua (e) -+ 0 in H - 1 (f~), and the proof is complete when

only body forces are considered. (ix) Let X ( f ~ ) ' = {v e L2(f~); Oar e L2(f~)} (Osv is a derivative in the sense of distributions). Then the trace v(., s) of any function v e X(f~) is well defined as a function in L2(w) for all s e [-1, 1] and the trace operator defined in this fashion is continuous. In particular, there exists a constant c4 such that 2

2

1/2

for all v C X(f~); as a consequence, there exists a constant c5 such that

IlvsllL,(r+ur_)

< cs ~ leillj(e; V)lo, f z .

.

for all v E V(ft) (these inequalities will afford the consideration of

surface forces in part (x)):

220

[Ch. 4

Linearly elastic elliptic membrane shells

Let v e X(f~). For almost ally e co and alls C [-1, 1], we can write (Ex. 4.1)

v(y, - 1 ) - v(y, s ) -

F

Osv(y,z3) dz3.

1

Consequently, Iv(.,-1)12,

0,

u e . a , e dz~ -~ {aa a in H i ( w ) as s --+ 0, e a,-

_ _

2s and

s - ~3 and thus ~ a 3 -

~3a 3 in L2(w) for all e > O,

If_': -

28

e

u~9 ~'~ dx~ --+ ~3a 3 in L2(w) as s --+ O.

Proof. As is easily seen (a similar a r g u m e n t was used in the proof of T h m . 3.3-1), the a s s u m p t i o n 8 E C3(~; I~3) implies t h a t the vector fields g a ( s ) 9~ -+ I~3 defined by 9 a ( s ) ( x ) "- 9 a'e (x ~) for all are such t h a t (the vector fields a n 9-~ -+ I~3 are identified here with vector fields defined over the set fl)" go(~)

-~o

o ( ~ ) i~ e ~ ( ~ ) .

-

Since

i F uen~o a'~ dx~

--

2~

e

-

~e

a

_

i F ~(~lg~(~l

~

d~s -

~~

I

= -

2

1

u ~ ( ~ ) ( g ~ ( ~ ) - a ~ ) e~3 - ( u ~ ( e ) -

~)a~,

232

Linearly elastic elliptic membrane shells

[Ch. 4

the convergences ua(e) ~ ua in Hl(fl) and ga(e) --4 a a in C1(~) imply that ua(e) (ga(e) - a a) -+ 0 in Hl(ft); hence 89f l 1 u a ( s ) ( g a ( s ) - a a) dza -+ 0 in Hi(w) by Thm. 4.2-1 (b). The same theorem also shows that ( u a ( e ) - ~ a ) a a -~ 0 in Hi(w). The proof is even simpler for the normal components" Since ga,6 = aa,

1;

2e

u~g 3,e dz i - ~ a 3 - (ua(e) - ~3)a 3

e

and Thm. 4.2-1 (a) then shows that (ua(e) - ~3)a 3 --~ 0 in L2(w). m The fields ~;" ~ --+ I~3 and ~ " ~T

: = i a~a

~

~ --+ I~3 defined by

a n d ~~~N ' - - i ~ a3,

which appear in Thm. 4.6-1, are respectively called the limit t a n gential d i s p l a c e m e n t field, and the limit n o r m a l d i s p l a c e m e n t field, of the middle surface S of the shell. Naturally, they are related to the limit displacement field ~e _ ~ai of S (Sect. 4.5) by

=

Under the essential assumptions that 70 = 7 and that the surface S is elliptic, we have therefore justified by a convergence result (Thm. 4.6-1) two-dimensional equations that are called those of a linearly elastic "membrane" shell in the literature (which, however, usually ig-

nores the distinction between "elliptic" and "generalized" membrane shells); see, e.g., Koiter [1966, eqs. (9.14) and (9.15)], Green & Zerna [1968, Sect. 11.1], Dikmen [1982, eqs. (7.10)], or Niordson [1985, eq. (10.3)]. In so doing, we have also justified the formal asymptotic approach of Sanchez-Palencia [1990] (see also Miara & Sanchez-Palencia [1996] and Caillerie & Sanchez-Palencia [1995b]) when "bending is well-inhibited", according to the terminology of E. Sanchez-Palencia. A w o r d of caution. In an elliptic membrane shell, body forces of order O(1) with respect to e thus produce a limit displacement field that is also O(1). By contrast, body forces must be of order O(e 2) in

Sect. 4.6]

Justification o/ the two-dimensional equations

233

order to produce an O(1) limit displacement field in a flezural shell. See Chap. 6. II The first convergence results for linearly elastic membrane shells have been obtained by Destuynder [1980] in his Doctoral Dissertation. In particular, the convergences established there in Thm. 7.9 (p. 305) under the assumption that the surface S is elliptic are almost identical to those established in Thm. 4.4-1 for the components ua(e), but "weaker" for the component u3(e), since P. Destuynder only established that eus(e) --+ 0 in L2(f~). Besides, his justification of the membrane shell equations remained partially formal as it still relied on an assumed asymptotic expansion of us(e). Using D-convergence theory (see, e.g., Vol. II, Sect. 1.11, and the references therein), Acerbi, Buttazzo gz Percivale [1988] were able to obtain convergence theorems for linearly elastic shells viewed as "thin inclusions" in a larger, surrounding elastic body. As a consequence, the distinction between membrane shells and flexural shells (Chap. 6) is no longer related to the geometry of the middle surface and to the boundary conditions as here, but instead to the ratio (as a power of e) between the Lam~ constants of the two elastic materials in presence. This asymptotic analysis is thus more reminiscent of that of Ciarlet, Le Dret & Nzengwa [1989] (described at length in Vol. II, Chap. 2), who considered an elastic multi-structure consisting of a plate partly inserted in an elastic body; if the shell were a plate, the approach of Acerbi, Buttazzo & Percivale [1988] would only apply to the inserted portion, however. After the original work of Ciarlet & Lods [1996b] described in this chapter, the asymptotic analysis of linearly elastic membrane shells underwent several refinements and generalizations: First, Genevey [1999] has shown that the convergence result of Thm. 4.4-1 can be also obtained by resorting to r-convergence theory. Using the techniques of Lions [1973], Mardare [1998a] was then able to compute a corrector, so as to obtain in this fashion the following remarkable error estimate: In addition to the hypotheses made in Thm. 4.4-1, assume that the boundary o/ the domain w is o~ class d 2, that Oaf a E L2(f~) and h i --O, and that

,f,

u dz~ e I-I2(w) r] VM(W).

234

Linearly elastic elliptic membrane shells

[Ch. 4

Then there exists a constant C -- C(w, 0, fi, ~) independent of e such that ]lu(~) - uliH,(n)•215

0 small enough and for all v E V(f~). Note that this inequality holds whether the space VF(w) reduces to {0} (as in this chapter or in Chap. 4) or not (as in the next chapter). Recall that another three-dimensional inequality of Korn's type holds, this time with a constant independent of e, but only for a family of elliptic membrane shells; cf. Sect. 4.3. A last preliminary is needed, in the form of the following definition (Sect. 5.5): The applied forces are said to be admissible if there exists a constant n0 such that

I{

,

,

z,3

for e > 0 small enough and for all v = (vi) E V(f~). Equipped with these preliminaries, we then establish the main result of this chapter: Consider a generalized membrane shell "of the first kind", i.e., one for which the space Vo(w) - { r / - (r/i) E Hi(w); rl - 0 on 70, 7,,~(r/) - 0 in w} "already" reduces to {0} (Sect. 5.4). [. [M defined by

Equivalently, the semi-norm

0,1

O,w a,/J

becomes a norm over the space V(od) -- { , :

(?]i) e Hi(w); r / = 0 on 70}.

This assumption is satisfied for instances if 70 ~ Ow and S is elliptic, or if S is a portion of a hyperboloid of revolution and 70 is "large enough" (these and other examples are reviewed in Sect. 5.8). We also assume that the applied forces are admissible. We then show (Thin. 5.6-1) that the averages 89f l 1 u(e) dx3 converge as e --+ 0 in the space V~M(f~) -- completion of V(w) with respect to I" IM,

244

[Ch. 5

Linearly elastic generalized membrane shells

and that the limit r C V~M(W) satisfies the following (scaled) twodimensional equations of a linearly elastic generalized membrane shell of the first kind: BL(r

r / ) - L~M(r/) for all r/C V~M(W),

where B L is the unique continuous extension to V~M(W) • V~M(W) of the bilinear form already encountered in the (scaled) two-dimensional variational problem of a membrane shell (Thm. 4.5-1), viz., (~, r/) e V(w) • V(w)-+ f~ aa~arT~r(~)Ta~(y)~dy , and the continuous linear form L~M 9V~M(W) ~ I~ reflects the limit behavior of the admissible applied forces as e ~ 0 (a convergence result also holds for the fields u(6) themselves; cf. again Thm. 5.6-1). We recall that ~(~)

~.~

1

-

~(0~o

_

4~,

+ 0o~) - ro~

~.,~

+ 2,(~.~,

- b~3,

~+

~.~~),

A+2/~ the functions 7a~(r/) and a a~ar being respectively the covariant components of the linearized change of metric tensor associated with a displacement field r/ia i of the middle surface S and the contravariant components of the (scaled) two-dimensional elasticity tensor of the shell. We also treat generalized membrane shells "of the second kind", i.e., tho~r fo~ winch L. lY i~ no longe~ a norm o~r

the space V ( ~ )

(this is simply another way of saying that V0(w) ~ {0}), but is a norm over the smaller space VK(~)-

{~ = (,~) e H~(~) • H~ ( ~ ) • H~(~);

r/i = 0~?s = 0 on 70} A convergence theorem can still be established in this case, but only in the completion of the quotient space V ( w ) / V o ( w ) with respect to I" IM (Thm. 5.6-2). We conclude this chapter by reviewing the existence and uniqueness properties of the solution to the above variational problem. We

Sect. 5.1]

245

Definition and assumptions on the data

also rewrite the fundamental convergence theorem in terms of descaled unknowns and data, thus providing a justification in terms of "physical" quantities of the two-dimensional equations of a linearly elastic generalized membrane shell (Thin. 5.8-1). These two-dimensional equations often provide intriguing examples of "sensitive" variational problems, according to the terminology recently introduced by J.L. Lions and E. Sanchez-Palencia, in the sense that they may possess two unusual features: They are posed in spaces that are not necessarily contained in spaces of distributions and their solutions may be "highly sensitive" to arbitrarily small smooth perturbations on the data (Sect. 5.8). In Sect. 5.8, we also review several examples of linearly elastic generalized membrane shells. 5.1.

LINEARLY ELASTIC GENERALIZED MEMBRANE SHELLS: DEFINITION AND ASSUMPTIONS ON THE DATA; THE THREE-DIMENSIONAL EQUATIONS OVER A DOMAIN INDEPENDENT OF g

Let w be a domain in It~2 with boundary 7 and let 8 E C2(~; R s) be an injective mapping such that the two vectors OaS(y) are linearly independent at all points y C ~. A linearly elastic shell with middle surface S = 8(~) is called a l i n e a r l y elastic g e n e r a l i z e d m e m b r a n e shell if the following three conditions are simultaneously satisfied (the definitions and notations are those of Sect. 3.1): (i) The shell is subjected to a boundary condition of place along a portion of its lateral face with 0(70) as its middle curve, where the subset 70 C 7 satisfies

length 70 > 0. (ii) Define the space (av denotes the outer normal derivative operator along 7):

vv(~) :--

{n-

(,7,) e H~(,,,) • n ~ ( , ~ ) • n ~ ( ~ ) ; r/i - 0,,~:3 - 0 on 70, 7a~(r/) - 0 in

w}.

Linearly elastic generalized membrane shells

246

[Ch. 5

Then vF(

) = {o}.

We recall that 1

tr

denote the covariant components of the linearized change of metric tensor associated with a displacement field yia i of the surface S. The subscript " F " announces the central rSle that the space VF(w) plays in the definition of flexural shells; cf. Sect. 6.1. (iii) The shell is not an elliptic membrane shell. We recall that a linearly elastic shell is an elliptic membrane shell if V0 - V and S is elliptic (Sect. 4.1) and that an elliptic membrane shell also provides an instance where the space VF(w), which in this case is the space H](w) • H~(w) • H2(w), reduces to {0} (if O e C2'1(w; Rz); cf. Thm. 2.7-2). Generalized membrane shells thus ezhaust all the remaining cases of l i n e a r l y elastic m e m b r a n e shells, i.e., those for which vF(

) = {o}.

Examples of linearly elastic generalized membrane shells are given in Sect. 5.8 A w o r d of c a u t i o n . Like the definition of a linearly elastic elliptic membrane shell, that of a linearly elastic generalized membrane shell depends only on the subset of the lateral face where the shell is subjected to a boundary condition of place (via the set V0) and on the "geometry" of the middle curve of the shell; cf. Ex. 5.1. i The formal analysis of Sect. 3.4 then naturally leads us to make the following scalings of t h e u n k n o w n s and a s s u m p t i o n s on t h e d a t a for a family of linearly elastic generalized membrane shells, with each having the same middle surface S = 0(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(V0) as its middle curve, as their thickness 2e approaches zero. First, we define the scaled u n k n o w n u(e) = (ui(s)) by letting

=.

-

e

Sect. 5.1]

247

Definition and assumptions on the data

Next, we require that the Lamd constants and the applied body and surface force densities be such that

and

#~ - #,

for all

x e -7r~x C ~2e,

for all

xe-Tr~xEr~_Ur

e

where the constants A > 0 and # > 0 and the functions f i C L2(~) and h i E L2(r+ U r_) are independent of e (Fig. 3.2-1 recapitulates the definitions of the sets f~e, f~, F~, r + , r e_, and r _ ) . Remark. For notational brevity, the functions fi and h i stand (as in the preceding chapter) for the functions that were respectively denoted fi, o and h i' t in Sect. 3.4. m

A w o r d of c a u t i o n . In order to carry out our asymptotic analysis of generalized membrane shells, we will have to make in addition a rather stringent assumption on the applied forces, which supersedes in fact the present ones, in such a way that the linear form appearing in the variational problem 7~(e; ~) described in Thm. 5.1-1 becomes continuous with respect to an ad hoc norm, and uniformly so with respect to ~; cf. Sect. 5.5. m As an immediate corollary to Thm. 3.2-1 (simply corresponding to p - 0), we obtain the problems satisfied by the scaled unknown over the set ~, thus over a domain that is independent of ~: T h e o r e m 5.1-1. Let w be a domain in R 2, let 0 E C2(~; ~3) be an injective mapping such that the two vectors aa - OaO are linearly independent at all points of-~, and let eo > 0 be as in Thm. 3.1-1. Consider a family of linearly elastic generalized membrane shells with thickness 2e, with each having the same middle surface S - 8(~) and with each subjected to a boundary condition of place along a portion o] its lateral face having the same set 8('/0) as its middle curve. Let the assumptions on the data be as above. Then, for each 0 < e ~ ~o, the scaled unknown u(s) - (ui(s)) satisfies the following s c a l e d t h r e e - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m :P(s; ~) of a

248

Linearly elastic generalizedmembrane shells

[Ch. 5

linearly elastic generalized m e m b r a n e shell: ~(8) C V ( ~ ) : = {~ = (~)i) E Hl(f~); v - 0 on to},

fflAijkl(g)eklll(8; ~(s))eillj(s; ~)r -- ff~ fir i ~ )

dx -~-fr

+UP-

dx

hil)i C g ( g ) d r

for all~ C V ( ~ ) ,

where ro "- 70 • [-1, 1], the scaled linearized strains eitlj(e; v) are given by

.)

-

1

+

-

e,~ll3(e;v) = ~l ( l oe 3 v ~ + c9,~v3)

P

(e)

p,

r:3(e)v~

eslls(e; v) = _103133, g and the functions AiJkt(e),

g(e), ri~(e )

are defined as in Thm. 3.2-1.

II Our main objective in this chapter consists in analyzing the behavior of the solutions u(e) C H I ( o ) of problems 79(e; f~) as e ~ O. To this end, we begin by proving in Sects. 5.2 and 5.3 various "analytical" preliminaries, which complement the "geometrical" and "mechanical" preliminaries proved in Sect. 3.3. Note that these preliminaries are common to all types of linearly elastic shells. In particular, they likewise play an essential r61e in the asymptotic analysis of linearly elastic flexural shells carried out in the next chapter. 5.2.

ANALYTICAL PRELIMINARIES

To begin with, we analyze the asymptotic behavior as e ---> 0 of the scaled linearized strains

Sect. 5.2]

249

Analytical preliminaries

appearing in the definition of the scaled three-dimensional problem T~(s; ~) (Thm. 5.1-1). To this end, we are naturally led to introduce the "three-dimensional analogs" Vaf~(v) and pa~(v) of the covariant components ~'af~(~) and Paf~(Y) of the "two-dimensional" linearized change of metric and change of curvature tensors (Sects. 2.4 and 2.5). The following result is due to Ciarlet, Lods & Miara [1996, Lemma 3.2]. T h e o r e m 5.2-1. Let the ]unctions r~a~, ba# , ~ ~ go (-~) be identified with functions in C~ and let for any v = (vi) C tI~(~2) the functions 7af~(v) ~ L2(~) and PaO(v) e H - ~ ( ~ ) be defined by: 7 . , ( ~ ) := 1 ( o ~ o + o ~ )

- r 7 ~ , ~ - bo..~,

p . , ( ~ ) := 0 . , , ~ - r ~ , o ~ +b~(0,,~

- r~.~)

+ b$(0.,~ - r ~ , . ) + ~1~

- ~7~,~,

~ h ~ b~lo - 0ob~ + r ~ b $ - r af3b~ ~ ~ - baif~ ~ (Thm. 2.5-1) Then there exists a constant Ct such that,/or all 0 < e ~_ ~o and all v E I-It(~), the scaled linearized strains ea{{f3(e; v) satisfiy 1 I~-~oll,(~; - ) - ~ ~l l , (~ ; -){0, . -< c ~ ~

I~o{0,., O~

where

1

1

and (11" I1-1,~ denotes the norm in H - I ( ~ ) ) : 1 0 3 ~ l l , ( ~ ; ~) + p ~ , ( ~ ) l i - ~ , n

Proof. The constants cl, c2 and c3 appearing in this proof are meant to be independent of e and of v C I-I1(~). The first inequality is a consequence of the definitions of the scaled strains Calif,(e; v) and of the asymptotic behavior of the functions riaf3 (~) (Tam. 3.3-1). Next, let the functions e~ v) e L2(~) and

250

[Ch. 5

Linearly elastic generalized membrane shells

tSaf~(v) e H - 1(12) be defined by

e~

,(

,

)

v ) : - - ~ tOotv3 Jr--oq3vc~ Jr-b~vtr, c ~a~(v) := Oaf3v3 + O~(b~vr) + O~(b~v~) - r ~ (O~v3 + 2b~v~)

-~;1~ - ~g~~. Then a simple computation shows that

0 (e ; V) - ba~e 3113(~; V) -b eX3 b~b~r~e3113(e; V) -2F,~%113 v) - OcrV3 - 2b~vr).

q-~x,3b~la(2e~

Consequently,

llO~llz,(~; v)§

,~,:,~(~,)ll-~,n

on the one hand. On the other, the first inequality implies that

11~1a=~,~l,~(~; v) - o=~,l~(~; v)ll-~,~ _< ~ ~ Ivalo,~, the definitions of the scaled strains eall3(e; v) and of the functions e~ v) together with the asymptotic behavior of the functions r~3(e ) imply that

le,:,l13(~; v)

o - ~oll=(~; ~)1o,~ _< ~3~ ~ I~1o,~,

and, finally, an easy computation shows that, for v E Hl(f~),

p~,(,,)- ~,~(,,). Hence the second inequality follows from the above relations.

II

The next theorem, which is due to Ciarlet, Lods & Miara Lemma 3.3], is crucial, as it plays an essential r61e in the of a three-dimensional inequality of Korn's type for a family early elastic shells (Thm. 5.3-1) and of the convergence of the

[1996, proofs of linscaled

Sect. 5.2]

Analytical preliminaries

251

unknown as e --~ 0 (Thms. 5.6-1 and 5.6-2): Consider a sequence (u(e))e>0 of functions in the space V(f~) that converges weakly in Ht(f~), thus also strongly in L2(f~), and let u be its limit. We first show that, if it so happens that the corresponding sequences (eillJ(e; u(e)))e>0 weakly converge in L2(f~), considerable information can then be gathered about the limit u and the functions 7a~3(u) and pa#(u). We also show that, if in addition the corresponding sequences (pa#(u(e)))e>o strongly converge in H-X(f~), then in fact the sequence (u(e))e>0 strongly converges in Ht(f~). In the following statement, the symbols -+ and ~ respectively denote strong and weak convergences and 0v denotes the outer normal derivative operator along the boundary of w. Theorem

5.2-2. Let v(~)

. - {~ - ( , , ) e a ~ ( u ) ;

~ - o on r 0 } ,

and let eillj(Z; "V) E L2(~), "/'a/3('V) E L2(~), and pa~('V) E I-]'-l(~) be defined for any function v E V(f~) as in Thms. 5.1-1 and 5.2-1. Let (u(e))~>0 be a sequence of functions u(e) E V(f~) that satisfies u(e) ~ u in Ht(f~), 1 -eeillJ(e; u(e)) --' elillj in L 2(f~), as e ~ O. Then u-

(ui) is independent of the transverse variable x3,

1//

-~ - ( ~ ) := ~

~ ~ d~3 e H ~(~) • H ~(~) • H ~(~),

ui -- 0~u3 - - 0 on 70, -y~(,,) - o,

pa,(u) E L2(n) and pa,(u)- -03e~ll,. If in addition there exist ]unctions Xa# E H-t(f~) such that p ~ ( ~ ( ~ ) ) -+ x ~

i~ a - ~ ( n )

~s ~ -~ o,

then .(~) -+.

i . r I l ( a ) ~s ~ -+ o,

pa~(u)- xa~ and thus Xa~ E L2(fl).

Linearly elastic generalized membrane shells

252

[Ch. 5

Proof. For the sake of clarity, the proof is divided into six parts, numbered (i) to (vi). We first recall that (Thm. 4.2-1 (a)), given v E L2(f~), ~ ( y ) : = 89f~i v(y, z3)dz3 is finite for almost all y E w and the average

1/:

-

V :-- "~

1

v dx3,

defined in this fashion is in L2(w), or in HI(w) if v E Hi(f~); in particular, the functions ~/are in H i (w) and they vanish on 70 (Thm. 4.2-1 (b)). For notational brevity, we let ei[ij(e ) --- eill:/(e; u(e)) throughout the proof. Finally, observe that the assumption u(~) --" u in Hl(f~) implies that u(e) --+ u in L2(f~) as the imbedding from Hi(f~) into L2(f~)is compact. (i) We first show that u - (ui) is independent of x3 and that - 0 on 70- Since the sequence (u(e))e>o is bounded in Hi(f~) and eillj(e ) --+ 0 in L2(f~) (in a Hilbert space, a weakly convergent sequence is bounded), 03u

(e) -

O u3(e) +

-

2rX3(

03u3(e) Hence 03Ui

"- 0,

in L2(~2), ce3113(c) -+ 0 in L2(f~). )u

-

(6)}

0

and consequently, by Thin. 4.2-1 (a),

u(y, x 3 ) - - ~ ( y ) for almost all (y, x3) e ~2, where the function ~ - (~/) = 89f_i i u d z 3 is in the space Hi(w) and satisfies ~ - 0 on 70. Thus u - (ui) is independent of the transverse variable z3. (ii) We next show that ~3 E H2(w) and Ov~3 v E Ci (~), an integration by parts shows that

0 on 3'0. If

17

x3v(y, z3) d$3 = -~

i (1 - x2)O3v(y, x3)dx3 for all y E ~.

By Thm. 4.2-1, the mappings w E L2(f~) ~ ~ E L2(w) and w E Hi(f~) -+ ~ E Hi(w)

Sect. 5.2]

253

Analytical preliminaries

are both continuous, so that the above relation remains valid (for almost all y E w) if v E Hi(f~). Let

1/:

~(~) - (~(~)) := ~ Hence we may also write

1;

~(~)- ~

(1 - x~)03u(s)dm3.

a:3U(~) dx3,

and, by Thm. 4.2-1 (b), ~i(s) E Hi(w) and ~i(s) - 0 on %. By assumption, e3[[3(e ) -- 103u3(~ ) ~

0 in L2(f~), and thus, by

definition of ~3i (s), The assumptions made on the sequence (u(s))e>0 combined with the asymptotic behavior of the functions r~3(s ) (Thm. 3.3-1) imply that 103ua(s)

-

2eall3(S)

-

O~u3(s) + 2 r ~ 3 ( s ) u ~ ( s ) ~

{-Oau3 2b~u~} -

in L2(f~), and thus (a strongly continuous linear mapping is also continuous for the weak topologies; see, e.g., Brezis [1983, Thm. III.9], by definition of ~ (~),

~(~)

1;

~

Since the functions again by Thm. 4.2-1 that -1 ~(~) -

(x~ -- 1)(Oau3 + 2b~u~)dx3 in L2(w).

u/ are independent of z3, since Oau3 = Oau3, (b), and since _~__f-ii (x 2 - 1)dx3 - 2,_ it follows -1 ~ := - ~2 (0a~3 + 2 ~ ~ )

in L2(w)

Our next objective consists in showing that, in ]act, the sequences (~(~))~>0 weakly converge in Hi(w). To this end, it suffices to establish that the sequences ( i ( o a ~ ( s ) + 0~l~ia(s)))e>0 weakly converge in L2(w) (by the two-dimensional Korn inequality, the norm I1" Ili,~ is equivalent to the norm (~?a) --~ {~-~a,~1 89 q- 0~Ta)l~,~} i/2 over

Linearly elastic generalized membrane shells

254

[Ch. 5

thespace {(r/a) E Hi(w); r/a - 0 on V0}). A simple computation, based in particular on the equality ~i(e) =

-

i

zSu(e) dz3, shows

that

-~ (oo~(~1 + o ~ ( ~ 1 ) - 2~~,,~(~) 2

",,~"

-

-

2babo.B;r,3"tt3(~) "4-

where ~ (~; eall/3(e) := eall~

(~) +

r~z=~

,,(~))

and the functions eall~(e; i v) are defined as in Thm. 5.2-1. The first inequality established in this theorem together with the assumptions us(g) --+ u s in L2(~) then imply that

1 } -+ o ~ii~(~)- ~li~(~)

in

.

(a),

1 i and the assumptions -chilD(s) --~ ealll 3 in L 2 (f~) in turn imply that g

e~ Ii,(e) ~ call i # in L2 (f~) Consequently, x3el,~ll~,e, ('~ --~ z3 elall~ in L2(W) Since u(e) ~ u in L2(f~) as u(e) ~ u in H i ( n ) by assumption, 2 (e))~>o and (bab~zsU3(e))e>o ~ 2 strongly conboth sequences (b~31az3u~ verge in L2(w); since ~ ( e ) ~ 0 in L2(w) (part (ii)), the sequence (ba#g~(e))~>0 strongly converges (to 0) in L2(w) and since (gza(e))e>0 weakly converges in L 2(w) (part (ii)), the sequence (ra/3u~(e))~>0~ -i weakly converges in L2(w). Hence the sequence (~za(e))e>0 weakly converges in Hi(w); thus ~za(e ) ~ ~ in L2 (w) implies that ~za e Hi(w), and therefore that 0a~3 E Hi(w) since ~ ~ E Hi(w); we have shown in this fashion that u3 E H2(w). We know from (ii) that ~ ( e ) - - 0 on 3'0; therefore, ~za(e ) ~ -"/.Sot i in Hi(w) implies that -~tct i _ 0 on 70. Since ui - 0 on 70, the equality ~1~. _ - 23( ~0 ., .~~ + 2bP.~..~.. shows that 0a~s - 0 on 70; hence

Ovu3 = 0 on 3'0. We have thus established that (ui) E H i ( w ) x H i ( w ) x H2(w) and that ~i = 0vu3 = 0 on 3'0.

Analytical preliminaries

S e c t . 5.2]

255

(iii) We ne=t prove that 7af3(u(e)) -+ 0 in L2(~) as s --+ 0 and that Va~(u) - O. By definition, the functions ealj~(s z ) are given by (Thm. 5.2-1) 1 Hence 1

I'ya/3(~(~))- e~ll/3(~)lo, n _< ~1er1

~e~ll/3(~)lo,~

and thus, by the first inequality in Thm. 5.2-1 and the assumptions made on the sequence (u(s))e>0,

7~(u(~)) -~ 0 i= L2(~). By the same assumptions, 7a~(u(s)) ~ Va~(u) in L2(I2). Hence Va~(u) - 0, as was to be proved. (iv) We next prove that paf~(u) = -03elallf~ in L2(fl). From the same assumptions and from the second inequality in Thm. 5.2-1, we infer that

{lo,~ll,(~) C

+

p~,(,,(~))} --~ o i~ H-~(a).

The operator 0a " L2(f~) --+ H-Z(f~) being also continuous for the weak topologies, we deduce from the assumption u(s) --~ u in HZ(I2) that _

103easlf3(s) ~

1 03Call ~ in H - 1 (f~),

hence that eaill3

~ 0 in H - (f~).

Since, again by the assumptions on the sequence (u(e))e>o,

256

Linearly elastic generalized membrane shells

[Ch. 5

the desired equality pa~(u) - -03e alll3 i holds in H - i (ft); that it is in fact an equality in L2(ft) follows from the relation ~3 E H2(w) established in part (ii) which, together with the independence of u3 with respect of z3 established in part (i), implies that u3 E H2(f~). (v) We ne~t prove that, under the additional assumption that p~z(u(e)) ~ x ~ in H - ~ ( n ) as ~ ~ O, the sequence (u3(r strongly converges in H i (f~). We first note that 03~t3(E) -- ~e3113(~) -+ 0 -- 03~t3 in L2(~).

By the lemma of J.L. Lions (Thin. 1.7-1), the mapping v E L2(~) -+ (v, (Oiv)) E H - I ( ~ ) x H - I ( ~ ) is an isomorphism. In order to prove that Oau3(e) -+ Oau3 in L2(~),

it therefore suffices to prove that

0~3(~) ~ 0~3 i~ H-~(~), 0aiU3(~ ) ---} OaiU3ill H-I(~'~).

The first convergence is a consequence of the assumed convergence u3(e) --+ u3 in L2(ft). The relation 03u3(~) --+ 0 = 03u3 in L2(ft) likewise implies that 0a3U3(~) --+ 0 -- 0a3U3 in H-i(f~).

From the definition of the functions Pat3(v) (Thm. 5.2-1) and from the assumption u(6) ---" u in I-Ii (f~), we infer that

p~z(,,(~)) -~ p~z(=) i= H-~(n), and thus,

p~(=(~)) -~ x~z - p~z(~) i= H-~(n). This relation also shows that Xat3 E L2(f~) since pa[3(u) E L2(~t)

(p~t (iv)). Since ui(e) --+ ui in H - i ( f t ) and Oaui(e) -+ Oaui in g - i ( ~ t ) by assumption, and since O~u3(e)

-

p ~ ( u ( e ) ) + r~,t30~u3(e ) - b~(O~u~(e) - r L = ~ ( ~ ) ) -bX(Oz=~(~)

-

r~=~(~)) - bXb=~(~) + bXbzu~(~),

257

Analytical preliminaries

Sect. 5.2]

the convergellces Oau3(e) ~ Oau3 in H - I ( ~ ) imply that

o~3(~)

~ o~3

i~ H-~(~).

Hence Oaiu3(e) --+ Oaiu3 in H-l(f~) and consequently,

Oau3(~) -+ Oau3 C L 2 ( ~ ) . (vi) Finally, we prove that the sequences (ua(e))e>o strongly converge in HZ(f~). By virtue of Korll's inequality applied to functions in the space V(f~), this is equivalent to proving that

eij(ut(e)) ~ eij(ut) ill L 2 ( ~ ) , where 1

~'(~) := (~(~), ~(~), 0),

U I := (~tl, ~t2, 0).

In part (iii), we have shown that 7a13(u(~)) -+ 0 in L2(n). Since

~.~(u'(~)) - v.~(u(e)) + r 2 ~ ( e ) + ba~u3(c), we conclude that eal3(ut(e)) ---+ { r ~ u t r

+ ba~u3} = ect~(U t) in L 2 ( ~ ) ,

by assumption. Next, 1

~ ( ~ ' ( ~ ) ) - ~o3~(~1 1

- ~e {2e~ 113(e) - O~u3(e) + 2r~3(e)u~(e)} --+ 0 - -~03u~ - e~3(u'),

-

by part (i); finally, e33(~t(c)) -- 0 -- e33(t/,'),

and the proof is complete.

II

258 5.3.

Linearly elastic generalized membrane shells

[Ch. 5

A THREE-DIMENSIONAL INEQUALITY OF KORN~S TYPE FOR A FAMILY OF LINEARLY ELASTIC SHELLS

The key to the convergence theorems of Sect. 5.6 is a three-dimensional inequality of Korn's type (Thm. 5.3-1), which may be viewed as a "scaled" Korn's inequality in curvilinear coordinates (Thm. 1.7-4) ]or linearly elastic shells. The "constant" C/6 appearing in this inequality, together with ad hoc assumptions on the applied forces (Sect. 5.5), will yield the fundamental a priori bounds that the family (u(c))s>0 satisfies (cf. parts (i) and (ii) in the proofs of Thms. 5.6-1 and 5.6-2). We emphasize that this inequality holds for an arbitrary "geometry" of the sur]ace S -- 8(~) and for an arbitrary subset "yo of 3~ with length V0 > 0, whether the space VF(w) introduced in Sect. 5.1 reduces to {0}, as in this chapter or the previous one, or not. Indeed, this inequality is likewise put to intensive use in the convergence theorem of the next chapter (Thm. 6.2-1)~ where we consider flexural shells, i.e., those for which Vv(w) ~ {0}.

Remarks. (1) We have seen in Thm. 4.3-1 that, if "Y0 = ~' and the surface S is elliptic, the "constant" C / s can be replaced by a "genuine" constant, i.e., that is independent of s; however, the norm Ilvslll, a appearing in the left-hand side must then be replaced by the norm I 10, (2) Another Korn inequality with a "constant" also of the form C//s was established in Kohn & Vogelius [1985] (see also Acerbi, Buttazzo & Percivale [1988]). It holds, however, over the "variable" domain f~ and besides, it involves the "usual" functions 89 (O~v~ + O~v~). II The following inequality of Korn's type is due to Ciarlet, Lods & Miara [1996, Thm. 4.1]; we recall that e0 > 0 is defined in Thm. 3.1-1. T h e o r e m 5.3-1. Assume that 8 E C3(~; I~S). Consider a family of linearly elastic shells with thickness 2e, with each having the same middle surface S : 0(-~) and with each subjected to a boundary condition of place along a portion of its lateral ]ace having the same

Sect. 5.3]

A three-dimensional inequality of Korn's type

259

set 0(7o) as its middle curve, where the subset 7o C 7 satisfies length 70 > 0. Define the space v(n)

: = {~ - ( , , ) e a ~ ( n ) ;

~ - o o. r0},

where Fo - 70 x [ - 1, 1]. Then there exist a constant ~1 satisfying 0 < el < so and a constant C such that, ]or all 0 < ~ < ~1, the following t h r e e -

d i m e n s i o n a l i n e q u a l i t y of Korn~s t y p e for a f a m i l y o f l i n e a r l y elastic shells holds:

~/2 Ilvlll~ < , _ - c { ~ l e.i l. l J ( ~ ; ~ v)l 2'n}

for all v C V(f~),

z~J

where the scaled linearized strains eillJ(e; v) are defined by

eol.,(~;

v) :=

1

~(0,vo + O.v,)- r:,(~)~.

e~lls(e; v) "= ~l(103va+Oav3) e

- r:~(~)~.

1 e3ll3(e; v ) :-- - 0 3 v 3 .

II Proof. Assume that this inequality is false. Then there exist em > 0 a n d v m - (vr~) e V ( f ~ ) , m - O , 1 , . . . (the Latin l e t t e r s m and n are used here for indexing sequences), such that

em -+ 0 as m - + cr 1 ~m

eillJ(em; v m) -+ 0 in L2(Ft) as m --+ c~.

Linearly elaztic generalized membrane shells

260

[Ch. 5

Since the sequence (Vm)mc~=O is bounded in H i ( ~ ) , there exist a subsequence ( v " ) ,oo = o and a function v E V(f~) such that v " ~ v in H i ( f ~ ) a n d v" ~ v in L2(f~)as n ~ c~.

Since

1 eallfl.(em; vm ) ~ 0 in L2(f~), em

10~eatlfl(e,; v n) --+ 0 in H - l ( a ) , gn

and, by the second inequality in Thin. 5.2-1,

+

1

v"

~n

_

)11 z,a

Hence the assumptions on the sequences (em)m~-_o and (v m)m~=o imply that We may thus apply Thm. 5.2-2. This gives: v - (vi) is independent of za,

-v - ( v i ) : =

1/:

~

i v dza E H i (w) • H i (w) • H 2 (w),

vi - Ovva - 0 on 70,

7af3(v) - pail(v) - 0 in ft. Consequently, 7af3 (v) - Pail (v) = 0 in w. The i n f i n i t e s i m a l rigid displacement l e m m a on a general surface (Thm. 2.6-3 (b)) then implies that ~ = 0 in w; hence v - 0 in fl since v is independent of xa. Thm. 5.2-2 also shows that v" -+ v in Hi(f~) as n --+ c~, so that v" --+ 0 in I-Ii(f~). But this contradicts [[v"l]i,a - 1 for all n, and the proof is complete, m If the mapping O is of the form 8(yl, y2) - (yi, y2, 0) for all (yi, Y2) E ~, the above inequality of Korn's type reduces for e - 1 to the t h r e e - d i m e n s i o n a l K o r n inequality in C a r t e s i a n coordinates over the set ~ = w • 1, 1[. m Remark.

Sect. 5.4] 5.4.

Generalized membrane shells of the first and second kinds

GENERALIZED MEMBRANE FIRST AND SECOND KINDS

261

SHELLS OF THE

According to the definition given in Sect. 5.1, if a linearly elastic shell is a generalized membrane shell, the space

VF(W) -- {W --(~7i) e HI(w) • HI(w) • H2(w); 7]i -- Or,~3 - - 0

on 7o, 7a~(17) - 0

in w)

reduces to {0). This condition is clearly equivalent to stating that

2

1/2

a,f~ for all ~1 - (Yi) e H i ( w ) • H i ( w ) • L2(w), becomes a n o r m over the space

v~(~)

:= {~ = (~i) e H~(~) • H~(~) • H~(~); r / / - O,,r/3 = 0 on 70 }.

The subscript " K " reminds that this space is central to the study of the two-dimensional Koiter equations for a linearly elastic shell; cf. Sect. 2.6 and Chap. 7. As already noted in Sect. 5.1, a linearly elastic elliptic membrane shell also provides an instance of such an occurrence since, by the inequality of Korn's type on an elliptic surface (Thm. 2.7-3), there exists a constant c such that 1/2

I1,o 1112,,,,+ J,~ 10,0,

< clv/IM for all v/E VM(w), --

O)

O~

where

v ~ ( . ~ ) . - Ho~(.~) • H~(~) • L~(~).

262

Linearly elastic generalized membrane shells

[Ch. 5

Hence if the shell is an elliptic membrane shell, the semi-norm I 9IM is already a norm over the space VM(W), thus a [ortiori over the space V g ( w ) , which in this case is equal to H~(w) x Hto(w) x H2(w). But this inequality of Korn's type shows much more, namely that the space VM(W) is complete when it is endowed with the norm I" !M (the "other" inequality clearly holds), a fact that sets elliptic membrane shells apart from generalized membrane shells. More specifically, the functional spaces in which the limit two-dimensional equations of a generalized membrane shell are well posed will turn out to be abstract completions, which are no longer immediately apprehensible! It seems in this respect that Destuynder [1985, p. 37] was the first to realize the need of considering such abstract completions in linearized membrane shell theory. As shown in the proof of the convergence theorem of Sect. 5.5, an additional precaution must be exercized, as generalized membrane shells need themselves to be subdivided into two different categories. To describe these, we introduce the two spaces v ( ~ ) .= {n = (v~) e E~(~); n = o o~ 70), v 0 ( ~ ) := {n e v ( ~ ) ; 7 ~ ( n ) = 0 i~ ~).

Remark. The space V0(w) thus plays the same r61e with respect to the space V(w) as does VF(w) with respect to r E ( w ) . In both cases, they constitute instances of spaces of "linearized inextensional displacements"; cf. Sect. 6.1. II Then a linearly elastic generalized membrane shell is of t h e first k i n d if

Vo(~) = {o), or equivalently, if the semi-norm 1" [M is "already" a norm over the space V(w) (hence a fortiori over the space VK(W) C V(w)). Otherwise, i.e., if

VF(w) = {0} but Vo(w)# {0}, or equivalently, if t 9IM is a norm over Vg(w) but not over V(w), the shell is a generalized membrane shell of t h e s e c o n d kind.

Sect. 5.4]

Generalized membrane shells of the first and second kinds

263

E z a m p l e s of linearly elastic generalized membrane shells of the

first kind abound; cf. Sect. 5.8. A w o r d of c a u t i o n . Whether a generalized membrane shell is of the first or second kind again depends only on the set V0 and on the "geometry" of the middle surface S; cf. Ex. 5.1. II An appraisal of the difficulties inherent to the analysis of generalized membrane shells lies in the definition of the ad hoc completions alluded to above: For a generalized membrane shell of the first kind, the limit two-dimensional equations are well posed in the space (Thm. 5.6-1) V~M(W) "-- completion of V(w) with respect to I" M, while for a generalized membrane shell of the second kind, these equations are well posed in the space (Thm. 5.6-2) V~M(W) := completion of v ( ~ ) / v 0 ( ~ ) with respect to I" MIdentifying such completions requires in each instance a careful analysis, which leads at times to surprising conclusions; the examples described in Sect. 5.8 are eloquent in this respect. Observe in this context how easier was the asymptotic analysis of a family of elliptic membrane shells, since V(w) - H01(w) in this case, so that the corresponding completion V~M(W) is simply the space -





To carry out our asymptotic analysis of a family of generalized membrane shells, we shall also need to consider the space (as usual, denotes the average of v with respect to the transverse variable) V0(12) : - {v E Hi(12); v - O on r0, Osv - O in 12, 7a~(v) - 0 in w},

which is the "three-dimensional analog" of the space V0(w). We shall likewise need the semi-norm I" IM defined by

iv12 .'-

2 + IO vlo,.

2}

for all v C V(12),

Linearly elastic generalized membrane shells

264

[Ch. 5

which is the "three-dimensional analog" of the semi-norm I" IM Observe in passing that 0g

"

Vo(.o) = {o) ~ Vo(n) = {o), or equivalently~ that l" IM i~ ~ ~o,m o~ the ~ p ~ v(~) if and only i f [ . IM is a norm over the space V ( ~ ) . In other words, a linearly elastic generalized membrane shell is of the first kind if and only if

Vo(a) = {o). 5.5.

ADMISSIBLE

APPLIED

FORCES

In order to derive the fundamental a priori estimates that the family (u(s))e>0 of scaled unknowns satisfies, we need to assume that the applied forces contribute in a special way to the variational problem T'(s; ~2)~ according to the following considerations. Consider a family of linearly elastic generalized membrane shells of the first or second kind, with thickness 2s, with each having the same middle surface S - 0(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(70) as its middle curve, and let the assumptions on the data be as in Sect. 5.1. For each s > 0, let the linear form L(s) : V ( ~ ) --+ R be defined by

L(~)(,,) .= fn

+uP_

for aU v E V(~2).

In other words, L(s)(v) is the right-hand side in problem :P(s; ~) (Thin. 5.1-1)~ which takes into account the applied forces through the functions ]i E L2(~) and h i C L2(r+ u r_). Then each linear form L(s) 9V(~2) -+ I~ is clearly continuous with respect to the norm I[" I!1,~ and uniformly so with respect to 0 < s ~ ~o (recall that g(s)(x) 0 functions FiJ(s) - FJi(s) E L2(f~) and there exist functions F ij = F ji E L2(f~) such that

- fn for aU 0 < s _< so and for all v E V(f~),

FiJ(e) --~ F ij in L2(~) as s ~ 0.

266

Linearly elastic generalized membrane shells

[Ch. 5

If the applied forces are admissible, there thus exists a constant n0 such that (recall that g(e)(x) < gl, x E ~; cf. Thm. 3.3-1)"

i,j

for all 0 < e _< e0 and for aU v C V(~2). As announced supra, this inequality will be put to an essential use in part (ii) of both Thms. 5.6-1 and 5.6-2.

Remark. The more convenient definition of admissible forces given here, which is due to Mardare [1998c], slightly differs from that originally given by Ciarlet & Lods [1996d]; cf. Ex. 5.2. 1 This definition is in effect an assumption about the contravariant components f~'e E L2(~ e) and h ~,e E of the applied body and surface forces actually acting on the shells of the family under consideration: It means that the right-hand side in the variational equations of problem ~(~e) (Sect. 3.1) can also be written ]or each

~>Oas

f~e

f$1 ev ie ~ / ~

d x e -4-

-

+ur 9 ~_

where vi(x) "- v~(x e) for all x e - 1rex e ~6 and L(e)(v) is of the above form. As such, it may be again understood as an assumption on the orders of the applied forces as 6 -+ 0. Naturally, admissible forces have to be identified for each type of generalized membrane shells; see in this respect the examples described in Sect. 5.8. 5.6.

C O N V E R G E N C E OF T H E S C A L E D D I S P L A C E M E N T S AS g --+ 0

We now establish the main results of this chapter: To begin with, we consider a family of linearly elastic generalized membrane shells o] the first kind, with thickness 2e > 0, with each having the same middle surface S = 8(W) and with each subjected to a boundary condition of place along a portion of its lateral face having the same

Sect. 5 . 6 ]

Convergence of the scaled displacements as e --4 0

267

set 0(V0) as its middle curve. Then the solutions u(e) of the associated scaled three-dimensional problems T'(e; [2) (Thm. 5.1-1) converge in an "abstract" completion V~M(~2) as e -+ 0. In addition, the averages

~(~)

1/

2

u(e)dxs

1

of the scaled unknowns likewise converge in an "abstract" completion V~M(W) as e -+ 0 and their limit satisfies an "abstract" variational problem posed over the same space VUM(W). The functions 7af3(v/) and a a ~ r used in the next theorem respectively represent the covariant components of the change of metric tensor associated with a displacement field yia i of the surface S and the contravariant components of the (scaled) two-dimensional elasticity tensor of the "limit" shell. Hence the bilinear form BM defined in/ra is precisely that found in the scaled variational problem of a linearly elastic elliptic membrane shell (Thm. 4.5-1). We recall that e0 > 0 is defined in Thm. 3.1-1. For convenience, we recapitulate the definitions of some spaces and semi-norms appearing in Thm. 5.6-1 and its proof:

v(a)

- {~ - (,~) e I ~ ( a ) ;

103rIo,2 • "J- ([~lwM)2 1/2

IVI~

v(~)

~ - o o . r0 - -~o • [-1, 1]}, where ~ -

1

- {~ - (~i) e H~(~); ~ = 0 o~ ~o},

Io1~ -

{

~

17,~,~(~)1~,,,,

}~/~

9

Notice that the assumption that is central to this chapter, namely that VF(w) -- {0} (Sect. 5.1), is not needed until part (vi) of the proof. The following result is due to Ciarlet & Lods [1996d, Thm. 5.1]; only the proof had to be slightly modified to take into account the new definition of admissible applied forces given in Sect. 5.5. T h e o r e m 5.6-1. Assume that 0 C C3(~; I~3). Consider a family of linearly elastic generalized membrane shells of the first kind (Sect. 5.4), with thickness 2s approaching zero, with each having the same middle surface S = 0(-~), with each subjected to a boundary condition

268

Linearly elastic generalized membrane shells

[Ch. 5

of place along a portion of its lateral face having the same set 0(')'0) as its middle curve, and subjected to applied forces that are admissible (Sect. 5.5). Let u(e) denote for 0 < e < eo the solution of the associated scaled three-dimensional problems 79(e; f~) (Thin. 5.1-1). Define the spaces

V~M(fl) "= completion of V(~t) with respect to l" IM, V~M(w) "-- completion of V(w) with respect to l" IM.

:=

1;

u(e) -+ u in V~M(f~) as e --+ 0, u(e) dx3 -+ r in V~M(w) as e -+ 0.

Let 4,~1~ aaf3a~ r , + 2p(aa~af3 r + a ~ a ~ ) ,

a a ~ ~ .__

)~+2p

1

7 ~ ( ~ ) "- i(0Z~. + 0o~Z) - r,zn~ - b,z~3, BM(r n) "- f~ a " Z ~ ~ ( r

fo~ r n e V(~), for n e V(w),

LM(rl) "= L ~~

1

A+2#

where the functions F ij C L2(f~) are those used in the definition of admissible forces (Sect. 5.5), and let B~M and L~M denote the unique continuous extensions from V(w) to V~M(W) of the bilinear form BM and linear form LM. Then the limit ~ satisfies the following sealed

two-dimensional variational p r o b l e m 7~M(W) of a linearly elastic generalized m e m b r a n e shell of the first kind: r E V~M(w) and B~M((, 1/) - L~(r/) for aU 7/E V~M(w).

Sect. 5.6]

Convergence of the scaled displacements as s ---> 0

269

Proof. The proof is divided into eleven parts. Throughout the proof, we let

~llj(~) := e~ll~(~; u(~)), and we let -~ and ~ respectively denote strong and weak convergences. Whenever Cl, c2, etc., appears in an inequality, it means that there exists a constant, denoted by this symbol, that is > 0 and independent of all the "variables" entering the inequality such that this inequality holds. (i) There exist 0 < el 0 in C~ 3.3-1) and the convergences (parts (vi) and (vii)) seall3(s ) --+ 0 in L2(~),

~u~(e) -~ o in L2(n), imply that

(Thm.

Sect. 5 . 6 ]

Convergence of the scaled displacements as e --+ 0

281

this shows that 0su' (e) --+ 0 in H - 1(f~). In view of establishing that eij(O3u'(e)) --+ 0 in H-l(f~), we first notice that ~s(os,,'(~))

= o3~ss(~,'(~))

= o.

The asymptotic behavior of the functions r~,s(e ) (Thin. 3.3-1) and the convergences eillJ(e) -4 eillJ in L2(f~) (part (vii)) next imply that {03Uct(g ) "4- e0c~t3(g) -}- 2~bXu~(e) } --4 0 in Z2(n); consequently O33ua(e) -1- eOa3u3(e)

-t-

2eb~,O3uo.(e) ~ 0 in H - l ( f l ) .

Since 03u3(e) --+ 0 in L2(f~) (part (ii)) and eu,,(e) ~ 0 in L2(f~) (part (vi)), we have

2eas(Osu'(e))

-

Ossua(e) --+ 0 in H-1(~2).

From the relations ealll3(e) --+ Call/3 in L2(~2) and 0seall/3 - 0 (part (vi)), we next infer that 03eall/3(e) --+ 0 in H - I ( ~ ) , hence that

{Osea~(u(e))-03( r pa~(e)up(e))} --~ 0 in H -1 (~), by definition of the functions eall/3(e). Because the functions rPa/3(e) are in cl(-~), the functions rPa~(e)Up(e) are in HI(~); besides,

o~(r~z(~)=~(~))

-

(o~r ~~z(~))=~(~)+ r ~~

(~)os~(e),

and c#3

since 03up(e) ~ 0 in H-~(f~) (we have established that 03U3(g) ~ 0 in L2(f~) in part (ii) and we just established that 03ua(e) ~ 0 in H-l(f~)). Finally, the estimates 11o3r~(~)llo,~,~ < c ~ (Thm. 3.3-1) and the convergences eu(e) --+ 0 in L2(ft) (part (vi)) imply that

(o~r~(~))~,(~) -~ 0 i~ L~Ca).

We thus infer from these relations that

and all the required convergences eij(O3u'(e)) -~ 0 in H-I(~) are thus established.

282

Linearly elastic generalized membrane shells

[Ch. 5

(xi) The whole family (u(e))e>0 converges strongly to u in the space V~M(~). We have shown that the whole family (u(s))e>0 converges in the space V~M(W) (part (viii)) and that Osu(6) --+ 0 in L2(~) for a subsequence (parts (ii) and (x)). Since the limit of this subsequence is unique, the whole family (Oau(s))e>o converges in L2(~). Hence the family (u(s))e>0 is a Cauchy sequence in the Hilbert space V~M(~), and the proof is complete. 1 Remark. Thm. 5.6-1 applies afortiori to a family of linearly elastic membrane shells, in which case the space V~M(W) is simply H~(w) • H~(w) • L2(w). The convergence obtained in this fashion "over the set w" is identical to, but the convergence "over the set fl" is weaker than, that obtained in Thm. 4.4-1, where we were able to establish the convergence of the family (u(e))e>0 in the space H I ( ~ ) • H I ( ~ ) x L2(~). In addition, we did not have to assume in Thm. 4.4-1 that the forces were "admissible". 1

We next consider a family of linearly elastic generalized membrane shells of the second kind, in which case similar convergences hold, again in "abstract" completions, but these are now completions of quotient spaces. We use the following notations: The equivalence class of v E V(~) in the quotient space V ( ~ ) / V 0 ( ~ ) is noted/~; likewise, the equivalence class of ~ e V(w) in the quotient space V ( w ) / V o ( w ) is noted/1. Similar notations designate equivalence classes in the completions The foUowing result is due to Ciarlet & Lods [1996d, Thm. 5.1]. T h e o r e m 5.6-2. Assume that 0 E C3(~; R3). Consider a family of linearly elastic generalized membrane shells of the second kind (Sect. 5.4), with thickness 2e approaching zero, with each having the same middle surface S - O(-~), and with each subjected to a boundary condition of place along a portion o] its lateral face having the same set 8('/0) as its middle curve, and subjected to applied forces that are admissible (Sect. 5.5). Let u(e) denote for 0 < ~ ~_ ~o the solution of the associated scaled three-dimensional problems :P(e; ~) (Thm. 5.1-1).

Sect. 5.6]

Convergence of the scaled displacements as e -~ 0

283

Define the spaces V~M(f]) "-- completion of V(f~)/V0(~t) with respect to [-[M, V~M(W) "-- completion of V(w)/Vo(w) with respect to l" IM

where Vo(~2) := {v E V(ft); 03v - 0 in f/, %t3(~)= 0 in w} # {0}, Vo(w) := {I/E V(w); %t3(~/)- 0 in w} # {0}.

Then there exist it E V~M(~) and ~ E ~r~M(W) such that /,(~) ~ / ,

in V~M(ft) as 6 -+ 0,

u(e) dz3 --+ ~ in V~M(w) as e --+ O.

Let the forms BM and LM be defined as in Thm. 5.6-1.

r

For

o E

/3M(~, //) := BM(~', rl') for any r E ~ and any r/' E//, LM(//) := LM(rI') for any r/' E//,

bilinear form BM and linear form s from V(w)/Vo(w) to ~flM(W). Then the limit ~ satisfies the following scaled t w o - d i m e n s i o n a l variational p r o b l e m 7~(w) of a generalized m e m b r a n e shell of the second kind-

284

[Ch. 5

Linearly elastic generalized membrane shells

Proof. The proof closely follows that of Thm. 5.6-1. We simply indicate which parts need to be modified.

Part (ii) becomes (otherwise its proof is identical)"

The semi-

.o~m~ I"(~)lg . . d I"(~)!~, h e . ~ th~ .o~m~ la(~)l.~ . . d la(~)l.~ and the norms ]leu(e)iil, a and ]eillJ(e)lo, n , are bounded independently

o/O0 is a Cauchy sequence with respect to the norm I" IM. By definition, -

= ~ a,~

=

-

I~(~(~11 -~.~(~(~'111~,~ + ~

10~,(~) - o~(~'11~,.. i

The remainder of the proof of part (x) is the same. Finally, part (xi) and its proof become: The whole/amily (u(e))e>0 converges strongly to it in the space ~r~M(f~). We have shown that the whole family (uie))e>o converges in the space ~r~M(W) (part (viii)) and that 03u(e) --+ 0 in L2(~) for a subsequence (parts (ii) and (x)). Since the limit of this subsequence is unique, the whole family (03u(e))e>o converges in L2(~2). Hence the family (u(~))e>o is a Cauchy sequence in the Hilbert space ~r~M(~2), and the proof is complete. II A scrutiny of the proofs of Thms. 5.6-1 and 5.6-2 shows that they provide worthy information about the asymptotic behavior of the scaled three-dimensional solutions u(e) and of their averages u(e), viz.

eillJ(e; u(e)) -+ eillj in L2(~),

os,,(~) ~ o in L(~), ~,(~) ~ 0 in tt~(~).

Sect. 5.7]

The two-dimensional equations

287

A noticeable feature of these convergences is that they occur in spaces that are more "decent" that the somewhat "exotic" spaces V~M(W) For a family of linearly elastic elliptic membrane, or flezural, shells, the three-dimensional limit u was, or will be, found to be independent of ~3 (Thms. 4.4-1 or 6.2-1). The convergence 03u(e) -~ 0 in L 2(f~) is an attenuated form of this property for a family of generalized membrane shells.

5.7.

T H E T W O - D I M E N S I O N A L E Q U A T I O N S OF A LINEARLY ELASTIC GENERALIZED M E M B R A N E SHELL; E X I S T E N C E A N D U N I Q U E N E S S OF S O L U T I O N S

For brevity, we only consider in this section generalized membrane shells of the first kind, as those of the second kind are treated in a similar fashion. The next theorem recapitulates the definition and assembles the main properties of the limit two-dimensional problem found at the outcome of the asymptotic analysis carried out in Thin. 5.6-1.

T h e o r e m 5.7-1. Let w be a domain in IR2, let 70 be a subset of the boundary of w with length 70 > 0, and let 8 e C3(~; IR3) be an injective mapping such that the two vectors aa -- Oa8 are linearly independent at all points of ~. Assume that Vo(~)

=

{o}, wh~

v 0 ( ~ ) := {~ = (~) e H~(~); ~ = o o~ ~0, ~ ( ~ ) 1 ~o~(~) .= ~ ( o ~ o + o o ~ ) - r ~ ~ - bo~3,

= 0 i~ ~},

and define the spaces

V(w) "= { ~ / - (Yi) E Hi(w); 17 = 0 on 70}, V~M(W) "-- completion of V(w) with respect to [. ]M, where

a, fl

Linearly elastic generalized membrane shells

288

[Ch. 5

Let aaf3ar ._ _

BM(r

U) ' =

4)~lZ aaf3aar + 2D(aaaaf3r + aaraf3~), A+2~

L ~"~~(r

~o~ r U e V(~).

L(U) "- f V ~ . ~ ( u ) ~ d y ~o~ U e V(~). J~

where the functions qoa# E L2(w) ave given, and let B~M and L~M denote the unique continuous extensions from V(w) to V~M(W) of the bilinear form BM and linear form L. Then the scaled two-dimensional variational problem 7)~M(W) of a linearly elastic generalized membrane shell of the first kind: Find that satisfies r C V~M(w) and B~M(r y) = L~M(y) for all y E V~M(w),

has one and only one solution. Proof. The assumption V0(w) = {0} means that the semi-norm [. ]M is a norm over the space V(w). The linear form L 9V(w) --+ R and the bilinear form BM : V(w) • V(w) --+ Ii~ are clearly continuous with respect to this norm. Besides, BM(~, ~)~_ cel v:~(l~l M ) 2 for all rl C V(w), since the scaled two-dimensional elasticity tensor of the shell is uniformly positive definite (Tam. 3.3-2 (a)) and a(y) > a0 > 0 for all y E ~ (Thm. 3.3-1). These properties remain valid on the space V~M(W) since V ( w ) i s by construction dense in V~M(W), again with respect to I" ]M~ . The conclusion thus follows from the La~-Milgram lemma. I Thm. 5.7-1 is established under the assumption that V0(w) = {0}. Therefore it applies not only to generalized membrane shells but also to elliptic membrane shells, since these satisfy the even stronger assumption (established in Thm. 2.7-2; recall that 70 = "Yin this case): {,I - (,7~)e H~(~,) • Ho~(~,) • L2(,,); "y~(,7) = o i~ ~,} - {o}.

Sect. 5.7]

289

The t w o - d i m e n s i o n a l equations

However, Thm. 5.7-1 alone does not say anything about the corresponding space V~M(W), which in this case turns out to be the space VM(W) -- H~(w) • H~(w) • L2(w). To prove this constitutes the "hard" part of the analysis, which rests on the inequality of Korn's type on an elliptic surface (Thm. 2.7-3). The same inequality is also crucially needed for establishing that, again in the case of an elliptic membrane shell, any continuous linear form L on the space VM(W) may be indeed expressed as in Thm. 5.7-1 by means of functions In order to get physically meaningful formulas, it remains to "descale" the unknown ~ that satisfies the limit "scaled" problem :P~M(W) found in Thm. 5.7-1. In view of the scaling -

-

-

e

made on the covariant components u~ of the displacement field (Sect. 5.1), we are naturally led to defining for each ~ > 0 the l i m i t v e c t o r field ~e by letting

A w o r d of c a u t i o n . For the elliptic membrane shells considered in the previous chapter, or for the flexural shells considered in the next chapter, each component of the field ~ = (~i) can be separately de-scaled, affording in turn the consideration of the limit tangential displacement field ~ a a and of the limit normal displacement field e 3 ~3a of the middle surface of the shell, where ~ := ~i (rE Sect. 4.6 or 6.4). By contrast, such a componentwise de-scaling is impossible for a generalized membrane shell, unless specific knowledge on the components of the "functions" in the completion V~M(W) allows to do so (the examples of Sect. 5.8 are particularly illuminating in this respect). In other words, the above de-scaling ~e = ~ is to be understood as an equality in the "abstract" completion V~M(W) and nothing else! 1 Recall that )e and #e denote for each e > 0 the actual Lam6 constants of the elastic material constituting the shell. We then have the following immediate corollary to Thm. 5.7-1; naturally, the existence and uniqueness results of Thm. 5.7-1 apply verbatim to the de-scaled problem T'~(w) (for this reason, they are not reproduced here)"

290

[Ch. 5

Linearly elastic generalized membrane shells

T h e o r e m 5.7-2. Let the assumptions and definitions not repeated here be as in Thm. 5.7-1, let aa/3'Tr, e ._.-- 4Ae# e aa/3a,Tr + 2l.te(aaaaf3r + aaraf3~r), A e + 2p e

Bi~(r V) := e f~ a " ~ " % ~ r ( r

for r

e V(~o).

L%(.7) := f~ ~o"~'~-y.~(.)~ey f o ~ . e v(~o). ~oar e := e~oa~, ~e I~e and let B M and L M denote the unique continuous extensions from V(w) to V~M(W) 4 the bilinear form B ~ and linear form L~M. Then the limit vector field ~e satisfies the following two-dimensional vari-

ational p r o b l e m 79~(w) of a linearly elastic generalized m e m b r a n e shell of the first kind: ~e ~, .) r e V~M(w) and BM(r

- L~

(.) for all

r/

e V~M(W).

Equivalently, the field ~e satisfies the following minimization problem:

~e E V~M(w) and j ~ ( ~ e ) _

inf.

Jg(,7) := II Each one of the two formulations found in Thm. 5.7-2 constitutes the two-dimensional equations of a linearly elastic generalized m e m b r a n e shell of the first kind. The functional j ~ . V~M(W) ~ R is the two-dimensional energy, and the functional 1 ~e-

is the two-dimensional strain energy, of a linearly elastic generalized m e m b r a n e shell of the first kind. The functions a a/3~T,e

Justification of the two-dimensional equations; ezamples

Sect. 5 . 8 ]

291

are the contravariant components of the t w o - d i m e n s i o n a l elasticity t e n s o r of t h e shell, already encountered in the two-dimensional equations of a linearly elastic elliptic membrane shell (Thm. 4.5-2). ~e Observe that the bilinear form B M found in the variational equations of a linearly elastic generalized membrane shell is an extension of the bilinear form B ~ already found in the variational equations of a linearly elastic elliptic membrane shell (Thm. 4.5-2). This is why both kinds constitute together the linearly elastic "membrane" shells. 5.8.

JUSTIFICATION OF THE TWO-DIMENSIONAL EQUATIONS OF A LINEARLY ELASTIC GENERALIZED MEMBRANE SHELL; EXAMPLES, COMMENTARY, AND REFINEMENTS

It remains to convert in terms of de-scaled unknowns the fundamental convergence result established in Sect. 5.6. As the "original" unknowns u ~ - (u~) are defined over a domain that varies with e (the set f~e), their averages 2~ fe-e u~ dz~ are more appropriate for this purpose, since they are defined over a fixed domain (the set w). For simplicity, we only consider generalized membrane shells of the first kind. T h e o r e m 5.8-1. Assume that 0 E C3(~; IR3). Consider a family of linearly elastic generalized membrane shells of the first kind (Sect. 5.4), with thickness 2~ approaching zero, with each having the same middle surface S = 0(-~), with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(7o) as its middle curve, and subjected to applied forces that are admissible (Sect. 5.5). For each e > O, let u e e ttl(f~ e) and Ce e V~M(W) respectively denote the solutions to the three-dimensional and two-dimensional

problems 79(f~e) and 79~(w) (Sect. 3.1 and

Thm. 5.7-2). Finally, let r e V~M(W) denote the solution to problem 7~M(W) (Thm. 5.7-1), which is thus independent of e. Then

~-~

1#

and ~

e

292

Linearly elastic generalized membrane shells

[Ch. 5

Proof. It suffices to combine the convergence

1; 2

1

established in Thm. 5.6-1, the relation

-

-

2s

e

u e dx~ - 1 -2

u(e) dx3, 1

which follows from the scaling u(s)(x) := u e (x e) for all x ~ - 7: x e Os (Sect. 5.1), and the de-scaling ~e := ~ (Sect. 5.7). II Remark. Without any specific information about the structure of the vector fields in the space V~M(W), these relations can no longer be refined (as in Sect. 4.6 for elliptic membrane shells) into ones involving separately the tangential and normal components of the three-dimensional displacement vector fields. II Under the essential assumptions that the space VF(W) reduces to {0) and that the forces are admissible, we have therefore justified by a convergence result (Thm. 5.8-1) the two-dimensional equations of a linearly elastic generalized membrane shell. In so doing, we have also justified the formal asymptotic approach of Caillerie & SanchezPalencia [1995b] when "bending is badly-inhibited", according to the terminology of E. Sanchez-Palencia. The asymptotic analysis of Ciarlet & Lods [1996d] described in this chapter has been extended by Slicaru [1998] to linearly elastic shells whose middle surface "has no boundary", such as a torus. Among linearly elastic shells, generalized membrane shells possess distinctive characteristics that set them apart: While forces applied to a family of elliptic membrane or flexural shells can be arbitrary (Sects. 4.1 and 6.1), body forces (for instance) applied to a family of generalized membrane shells can no longer be accounted for by an arbitrary linear form of the form v i v/fig dx ~, i.e., with arbitrary contravariant components fi,~ E L2(12~). They must be admissible "for the three-dimensional equations", in order that the associated scaled linear forms be continuous with respect to the norm v --+ { ~ i , j leillJ(6; v)l~,~} 1/2 and uniformly so with respect to s > 0 (Sect. 5.5).

Sect. 5.8]

Justificationof the two-dimensional equations; e~amples

293

The linear form found in the variational equations of the limit two-dimensional problem for such a shell is likewise subjected to a restriction: On the dense subspace V(w) of the space V~M(W), it must be of the form ~/--~ f~ 7~a~3'a~(r/)V~ dy (Thm. 5.6-1). In other words, the applied forces must be also admissible "for the two-dimensional equations "~ in such a way that the linear form appearing therein must be an element of the dual space of V~M(W). As this dual space may be quite "small'~ the limit variational problem, which otherwise satisfies all the assumptions of the LaxMilgram lemma (Thm. 5.7-1)~ possesses the unusual feature that its solution may no longer exist if the data undergo arbitrarily small, yet arbitrarily smooth, perturbations! Another unusual feature of this problem is that the space V~M(W) in which its solution is sought may not necessarily be a space of distributions! Such variational problems fall in the category of "sensitive problems" introduced by Lions & Sanchez-Palencia [1994]. Since then, such problems have been extensively studied~ either for their own sake or as regards their relations to the theory of generalized membrane shells, by Lions & Sanchez-Palencia [1996, 1997a, 1997b, 1998], Pitk/iranta & Sanchez-Palencia [1997], Sanchez-Palencia [1999], LeguiUon, Sanchez-Hubert & Sanchez-Palencia [1999]. Ezamples of linearly elastic generalized membrane shells are numerous. In each case~ however, the proof that the space VF(w) reduces to {0} and the identification of the corresponding space V~M(W) and of the admissible applied forces usually require delicate analyses. For this reason, these are not given here; only ad hoc references are provided. A measure of the difficulty inherent to showing that VF(w) -- {0} is given by the proof of the infinitesimal rigid displacement lemma when the surface S - 8(~) is elliptic and 70 = 7 (Whm. 2.7-2). All the following examples correspond to V0(w) - {0}, i.e., to generalized membrane shells of the first kind~ according to the definition of Sect. 5.4.

Remark. It seems that there are no known examples of generalized membrane shells of the second kind. According to C. Mardare, they should correspond to surfaces S "with little regularity", m A first ezample is provided by a shell whose middle surface is a portion of an elliptic surface S -- 8(-~), i.e., one whose Gaussian

294

Linearly elastic generalized membrane shells

[Ch. 5

Fig. 5.8-1: Two linearly elastic generalized membrane shells. A shell whose middle surface S = 0(~) is a portion of an ellipsoid and which is subjected to a b o u n d a r y condition of place (i.e., of vanishing displacement field) along a portion (darkened on the figure) of its lateral face whose middle curve 0(7o ) is such t h a t 0 < length 7o < length 7, provides an instance of a linearly elastic generalized m e m b r a n e shell, i.e., one which is not an elliptic membrane shell (Chap. 4), yet whose associated space V F ( w ) = {W = (~/,) e Hi(w) x HX(w) x H2(w); 17i = 0~7/s = 0 on 70} contains only W = 0 (like that associated with an elliptic m e m b r a n e shell). A comparison with Fig. 4.1-1 illustrates the crucial rSle played by the set 0(70) for determining the type of a shell! A shell whose middle surface S = 0(~) is a portion of a hyperboloid of revolution and which is subjected to a b o u n d a r y condition of place along its entire "lower" lateral face provides another instance of a linearly elastic generalized m e m b r a n e shell.

curvature is everywhere > 0 (Sect. 4.1), and which is subjected to a boundary condition of place along a portion of its lateral face whose middle curve 0(70) is such that 0 < length 7o < length 7 (Fig. 5.81). Using the unique continuation theorem of HSrmander [1983], Lods & Mardare [1998a] have shown that, under the assumption that 0 E C2' 1(~; ]R3), the space "- {,7 - (Vi) e



• L2(o );

- 0 o n 7o,

"already" reduces to {0}; hence afortiori Vo(w) = {0}!

Sect. 5 . 8 ]

Justificationof the two-dimensional equations; ezamples

295

This result extends an earlier result of Vekua [1962] who had shown that It(w) = {0} under the assumptions that O E W3'P(w; I~3), p > 2, and that 7 is of class C3. It also contains in the special case where 3'0 = 3' the infinitesimal rigid displacement lemma on an elliptic surface (Thin. 2.7-2) due to Ciarlet & Lods [1996a] and Ciarlet & Sanchez-Palencia [1996]. The two-dimensional equations for such a shell constitutes an example of a sensitive problem: As shown by Lions & Sanchez-Palencia [1996], the space V~M(W) is not a space of distributions and there exist functions pi E :D(w) such that applied forces corresponding to the linear form ~1 --+ f~ Pi~Ti~ dy are not admissible for the two-dimensional equations! Lods & Mardare [1998a] have also shown that the regularity of the mapping 0 and the assumption of ellipticity of the surface S can be both substantially weakened when S is a portion of a surface of

revolution. Remark. While the space V~M(W) corresponding to an elliptic membrane shell, i.e., one whose middle surface S is smooth and elliptic and which is subjected to a boundary condition of place along its entire lateral face (7o = 7), is a space of distributions (since V~M(W) -- Hio(w) x Hio(w) • L2(w) in this case; cf. Chap. 4), it ceases to be so when there is a fold, also called an edge, on S, in which case the two-dimensional problem becomes sensitive; see Lions & SanchezPalencia [1998], G~rard & Sanchez-Palencia [1999]. I

A second ezample is that of a shell whose middle surface is a portion of a hyperbolic surface S, i.e., one whose Gaussian curvature is everywhere < 0, provided the curve intersects all the asymptotic lines (Sect. 2.2) of S; for instance, a shell whose middle surface is a portion of a hyperboloid of revolution and which is subjected to a boundary condition of place along its entire "lower" lateral face (Fig. 5.8-1) fulfills these requirements. Under the assumption that O E c2'l(w; ]~3), Mardare [1998c] has shown that R(w) = {0} and that the space V~M(W) is a closed subspace of L2(w) x L2(w) x H - i ( w ) , extending in this fashion earlier results of Vekua [1962] and Sanchez-Palencia [1993]. Interesting complements about shells with hyperbolic middle surfaces are found in Sanchez-Hubert gz Sanchez-Palencia [1997, Chap. 7, Sect. 2], Karamian [199Sb].

296

Linearly elastic generalized membrane shells

[Ch. 5

i j

Fig. 5.8-2: Other ezample8 of linearly elastic generalized membrane shells. Consider a shell whose middle surface S = 0(~) is a portion of a cone or a cylinder and which is subjected to a b o u n d a r y condition of place (i.e., of vanishing displacement field) along a portion (darkened on the figure) of its lateral face with O(')'0) as its middle curve. If O(V0) intersects all the generatrices of S, such a shell is a linearly elastic generalized membrane shell.

Remark. If the hyperbolic surface S has a fold, the space V~M(W) may no longer be a space of distributions, thus yielding another example of sensitive problem; see Lions & Sanchez-Palencia [1997b]. II

A third ezample is that of a shell whose middle surface S is a portion of a parabolic surface, i.e., one consisting entirely of parabolic points (Sect. 2.2), again if the set 0(~'0) is "large enough". Such is the case when S is a portion of a cylinder or a portion of a cone and the curve O(~fo) intersects all the generatrices of S (which are also the asymptotic lines of S in this case; cf. Sect. 2.2); cf. Fig. 5.8-2. Under the assumption that 8 E W2'~176 I~a), Mardare [1998c] has shown that It(w) - {0} and that the space V~M(W)is a closed subspace of H - l ( w ) • H - l ( w ) • H-2(w); the regularity assumptions can again be

Ezercises

297

weakened when S is a portion of a surface of revolution. Interesting complements about shells with parabolic middle surfaces are found in Sanchez-Hubert & Sanchez-Palencia [1997, Chap. 7, Sect. 4]. A compact surface "without boundary" is infinitesimally rigid if any displacement field satisfying Va~(~/) = 0 everywhere on the surface (these relations must be first re-interpreted so as to make sense on such a surface) are infinitesimal rigid displacements in the sense of Thm. 2.6-5. The identification of such infinitesimally rigid surfaces is a classical problem in the differential geometry of surfaces; see, e.g., Nirenberg [1962]. A shell whose middle surface S has no boundary is a linearly elastic generalized membrane shell if S is infinitesimally rigid. Such shells have been extensively studied by Slicaru [1998], who notably extended the analysis of Metskhovrishvili [1957] when S is a torus. A related phenomenon is the infinitesimal rigidification induced by folds on a surface and its relations with linear shell theory. In particular, the asymptotic behavior as the thickness approaches zero of a shell with a smooth middle surface and that of one with an arbitrarily close middle surface, but with folds (such as a polyhedral surface, i.e., an assembly of planar facets), may be startlingly different! In this direction, see Akian & Sanchez-Palencia [1992], Choi [1993], Choi & Sanchez-Palencia [1993], Geymonat & SanchezPalencia [1995], Sanchez-Palencia [1995], G~rard & Sanchez-Palencia [1999].

EXERCISES

5.1. The notations used in (1) should be self-explanatory. (1) Let a surface S -- 0(~) -- 0 ( { ~ } - ) be equipped with two systems of curvilinear coordinates (ya) C ~ and (ya) C { ~ } - and assume that 0(V0) - 0(V0). Show that Vg(w) - {0} implies that V F ( ~ ) - {0}. This means that the definition of a linearly elastic generalized membrane shell (Sect. 5.1) is independent of the system of curvilinear coordinates employed for representing the surface S. (2) Show that whether such a shell is of the first or of the second kind (Sect. 5.4) is likewise independent of the particular system of curvilinear coordinates employed.

298

Linearly elastic generalized membrane shells

[Ch. 5

5.2. According to the definition originally given by Ciarlet & Lods [1996d], the applied forces are admissible if, for each e > 0, there exist functions ~oaf3(s) - q~oa(s) e L2(w) and Fi(s) e L2(~) such that L ( e ) ( v ) may be also expressed as

dy + fn for all v E V(~2), where ~ = ~1 f_l 1 v dxa, and if there exist functions ~oafJ C L2(w) and F i E L2(~) such that ~oa/3(e) -+ ~oa/3 in L2(w) and Fi(e) -+ F i in L2(f~) as e --> O. Using this definition (which differs from that of Sect. 5.5), carry out an asymptotic analysis analogous to that of Thm. 5.6-1. Hint: If the applied forces are admissible, there exists a constant C such that (recall that g(e) - a + O(e) in C~ cf. T a m . 3.3-1). IL(e)(v)[ < C3[vl M for all v e V(~2) and all 0 < e _< e0.

For further details, see Ciarlet & Lods [1996d, Thm. 5.1].

CHAPTER 6 LINEARLY

ELASTIC

FLEXURAL

SHELLS

INTRODUCTION

Consider a linearly elastic shell with middle surface S = 8(~), subjected to a b o u n d a r y condition of place along a portion of its lateral face with 8(70) as its middle curve, where 7o C 7. Such a shell is a linearly elastic flezural shell if its associated space

v~(~)

- {~ - (,~) e H ~ ( ~ ) • H ~ ( ~ ) • H ~ ( ~ ) ; yi - 0~ya - 0 o n 7 0 , 7 a ~ ( ' 1 ) - 0 in w }.

contains nonzero functions (Sect. 6.1). Examples, where S is either a portion of a cylinder (in which case 8(70) is included in one or two generatrices) or a portion of a cone (in which case ~(70) is included in one generatrix) are presented in Sect. 6.1. The purpose of this chapter is to identify and to mathematically justify the two-dimensional equations of a linearly elastic flexural shell, by establishing the convergence in ad hoc functional spaces of the three-dimensional displacements as the thickness of such a shell approaches zero. More specifically, consider a family of linearly elastic flexural shells with thickness 2c approaching zero, with each having the same middle surface S = 8(~), and with each subjected to a b o u n d a r y condition of place along a portion of its lateral face having the same set 8(70) as its middle curve. The associated three-dimensional problems, posed in curvilinear coordinates over the sets 12~ = w x ] - c, el, are first transformed for each ~ > 0 into equivalent problems, but now posed over the set 12 = w x] - 1,1[, which is independent of e. This transformation relies in a crucial way on appropriate scalings of the unknowns u i (the covariant components of the displacement field) and assumptions on the Lamd constants )~ and #e and on the contravariant components fi, e of the applied body forces (for simplicity, we assume in this

Linearly elastic flezural shells

300

[Ch. 6

introduction that there are no applied surface forces). More specifically, we define the scaled unknown u(s) = (ui(s)) by letting

Zt~(Xe) -- 'tti(g)(X ) for all z" = ~r'z E ~ ' , where 7r~(xl, x2, x3) = (Xl, x2, sx3). We then assume that there exist constants A > 0 and/z > 0 and f u n c t i o n s / i independent of e such that Ae

= A

and pe

=/z,

f i " ( x ' ) -- s2fi(x) for all z e - ,fez E f~e. It is found in this fashion that the scaled unknown u(e) satisfies a variational problem of the form (Thm. 6.1-1):

u(s) --(ui(s)) E V ( ~ ) -

{v - ( v i ) E H I ( ~ ) ; v-

f

0 on Vo • [-1, 1]},

AiJkZ(s)ekllt(s; u(s))eillJ(~; v ) ~ - ( s ) d x = ~2 f f i v i % ~ ) d x gft

for aU v E V ( ~ ) ,

where, for any vector field v = (vi) E Hl(f~), the scaled linearized strains e~llj(e; v) - ejll~(e; v) E L2(n) are defined by:

-

1

p

+

l(103Va+Oav3)

-

e3113(e; v) - 103v3. g

Using various analytical preliminaries established in the previous chapter, most notably the three-dimensional inequality o] Korn's type /or a family of linearly elastic shells, we then establish the main result of this chapter (Thm. 6.2-1), by showing that the family (u(e))e>o strongly converges in the space H I ( n ) as s -+ 0 and that u = lime--+ou(s) is obtained by solving a two-dimensional problem.

301

Introduction

More specifically, we show that the limit u is independent of the transverse variable and that ~ = 89f l 1 u dx3 satisfies the following (scaled) two dimensional variational problem of a linearly elastic flex-

ural shell: r E V F ( W ) - { r / - (r/i) e HI(w) x Hi(w) x H2(w); r / i - 0vy3 - 0 on 70, Vaf3(r/)- 0 in w},

1 1 -~ f aat3~rpar(')Pal3(rl)~dY: f ~ { f l ' i d x a } ~ i x ~ d Y for all v / = (7//) e Vv(w), where

=

p~(r/) -

aaf3~r _

+

-

-

ba

73,

0~73 - F~#0,W3 - b~b~/3~73+ b~(Oarl~ - r ~ , ~ , )

4Ap aaf3a,Tr+ 2#(aaCaf3r + aara~r )~+2#

the functions 7a/3(v/), pal3(v/), and a a/3~r being respectively the covariant components of the linearized change of metric and change of curvature tensors associated with a displacement field r//a / of the middle surface S (first encountered in Sects. 2.4 and 2.5) and the contravariant components of the (scaled) two-dimensional elasticity

tensor of the shell. We conclude this chapter by reviewing the existence and uniqueness properties of the solution to the above variational problem and to the associated minimization problem (Thm. 6.3-1). We also rewrite the fundamental convergence theorem in terms of de-scaled unknowns and data, thus providing a justification in terms of "physical" quantities of the two-dimensional equations of a linearly elastic flexural shell (Thm. 6.4-1). In particular, the limit displacement field ~ a z of the middle surface S is such that ~e _ ( ~ ) satisfies the following minimization

problem: ~e e VF(w) and j ~ ( ~ e ) _

inf

j~(r/),

Linearly elastic flezural shells

302

[Ch. 6

where the two-dimensional energy j~ 9Vy(w) --+ I~ is defined by

1f

e 3aa~r'ep~r(rl)pa~(rl)~/-a dy

J~,

and 4A~#~ Ae

6.1.

+ 2p ~

~~

+ 2,~(~~ ~+ ~~).

LINEARLY ELASTIC FLEXURAL SHELLS: DEFINITION~ EXAMPLES, AND ASSUMPTIONS ON THE DATA; THE THREE-DIMENSIONAL EQUATIONS OVER A DOMAIN INDEPENDENT OF

Let w be a domain in I~2 with boundary V and let 0 E C2(~; I~3) be an injective mapping such that the two vectors OaS(y) are linearly independent at all points y E ~. A linearly elastic shell with middle surface S = 0(~) is called a l i n e a r l y elastic f l e x u r a l shell if the following two conditions are simultaneously satisfied (the definitions and notations are those of Sect. 3.1): (i) The shell is subjected to a boundary condition of place along a portion of its lateral face with 0(7o) as its middle curve, where the subset V0 C V satisfies

length 7o > O. (ii) Define the space (0~ denotes the outer normal derivative operator along 7)" VF(W) := { ~ -

(~i) 6 H i ( w ) x / - / l ( w ) x H2(w); Yi - 0vy3 - 0 on 70, 7a#(Y) - 0 in w}.

Sect. 6 . 1 ]

Definition, ezamples, and assumption on the data

303

Then the space VF(w) contains nonzero functions; equivalently,

vF( ) # {o). We recall that the functions 1

O"

denote the covariant components of the linearized change of metric tensor associated with a displacement field yia i of the surface S. The subscript " F " announces that VF(w) is the functional space over which the limit two-dimensional equations of a linearly elastic flexural shell are posed (Thin. 6.2-1). In other words, there exist nonzero a d m i s s i b l e l i n e a r i z e d inext e n s i o n a l d i s p l a c e m e n t s y i a i of the middle surface S: "Admissible" means that they satisfy boundary conditions "of clamping" along the curve 8(70), expressed here by means of the boundary conditions yi - Ouy3 on 70 on the associated field r / - (yi) (these boundary conditions are interpreted later; cf. Sect. 6.4); "linearized inextensional" reflects that the functions 7a~(r/) are the linearizations with respect to W -- (rli) of the covariant components of the exact change of metric tensor associated with a displacement field y i a z of the surface S; cf. Sect. 2.4. Examples of linearly elastic flexural shells are given in Figs. 6.1-1 to 6.1-3; see also Exs. 6.1 to 6.5. A w o r d of c a u t i o n . Like those of linearly elastic elliptic membrane or generalized membrane shells, the definition of a linearly elastic flexural shell depends only on the subset of the lateral face where the shell is subjected to a boundary condition of place (via the set 70) and on the geometry of the middle surface of the shell; in this respect, see also Ex. 6.6. m The formal analysis of Sect. 3.4 then naturally leads us to make the following s c a l i n g s of t h e u n k n o w n s and a s s u m p t i o n s o n t h e d a t a for a family of linearly elastic flexural shells, with each having the same middle surface S - 0(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(70) as its middle curve, as their thickness 2e approaches zero.

304

Linearly elastic flezural shells

[Ch. 6

/

Fig. 6.1-1: A linearly elastic flezural shell. A shell whose middle surface S = 8(~) is a portion of a cylinder and which is subjected to a boundary condition of place (i.e., of vanishing displacement field) along a portion (darkened on the figure) of its lateral face whose middle curve 8(70) is contained in one or two generatrices of S provides an instance of a linearly elastic flexural shell, i.e., one for which the space v.(~)

= ~ , ~ H~(~) • H~(~) • H~(~); ~, = o ~

= 0 o . ~o, ~ o ~ ( , ) = 0 i . ~}

contains nonzero functions ~/; cf. Ex. 6.1. The "two-dimensional boundary conditions of clamping" 7/i -- a~T/s - 0 on 70 inherited by the limit two-dimensional equations are so named because they mean that the points of, and the tangent spaces to, the deformed and undeformed middle surfaces coincide along the set 8(70) (as suggested in the "two-dimensional" figure); cf. Sect. 6.3. This example and that of the cylindrical shell from Fig. 5.8-2 illustrate the crucial rSle played by the set 8(7o) for determining the type of a shell.

Sect. 6 . 1 ]

Definition, ezamples, and assumption on the data

305

Fig. 6.1-2: Another ezample of a linearly elastic flezural shell. A shell whose middle surface S = 0(~) is a portion of a cone excluding its vertex and which is subjected to a boundary condition of place along a portion (darkened on the figure) of its lateral face whose middle curve 8(70) is contained in one generatrix of S provides another example where VF(w) r {0}; el. Ex. 6.2. The two-dimensional boundary conditions of clamping inherited by the limit two-dimensional equations are suggested on the "two-dimensional" figure. A comparison with Fig. 5.8-2 again illustrates the rSle played by the set 0(7o) for determining the type of shell.

u ( e ) = (ui($)) by l e t t i n g

F i r s t , we define t h e s e a l e d u n k n o w n

~Z~(Xe) --" Zti(8)(X ) for all x e - 7r~x C ~ . N e x t , we require t h a t the Lamd constants a n d t h e applied body and surface force densities be such t h a t

)~e = :k fi, e ( x c ) =

e2fi(x)

and

#e = / ~ ,

for all

x" - r e x

an

-

E f~e, c

u r'_,

where the constants ~ > 0 and # > 0 and the functions f i E L 2 ( ~ ) and h ~ E L 2 ( p + U r _ ) are independent of e (Fig. 3.2-1 r e c a p i t u l a t e s t h e definitions of t h e sets f~e f~, P~_, r

r e

and r_)

306

Linearly elastic flezural shells

[Ch. 6

t t x,~

..

Fig. 6.1-3: Another ezample of a linearly elastic flezural shell. A plate subjected to a boundary condition of place along any portion (darkened on the figure) of its lateral face whose middle line 70 satisfies length 70 > 0 provides an instance of a linearly elastic flexuxal shell since Vp(w) D ( r / = (0, 0, r/s); r/s E H~(w)) ~ ~0) in each case; cf. Ex. 6.3. The two-dimensional boundary conditions of clamping inherited by the limit two-dimensional equations are suggested on the "two-dimensional" figures (for visual clarity, only a portion of the plate is represented in the last case). Surprisingly, if 7o is "large enough", the same plate is no longer modeled as a flexuxal shell when it is viewed as a nonlinearly elastic body! See Fig. 9.1-2.

Sect. 6.1]

Definition, ezamples, and assumption on the data

307

Remark. For notational brevity, the functions f i and h i stand for the functions that were respectively denoted fi, 2 and h i' 3 in Sect. 3.4. II

As an immediate corollary to Thm. 3.2-1 (simply corresponding to p - 2), we obtain the problems satisfied by the scaled unknown over the set f~, thus over a domain that is independent o/e" T h e o r e m 6.1-1. Let w be a domain in IR2, let 0 E C2(~; IR3) be an injective mapping such that the two vectors aa = OaO are linearly independent at all points of-~, and let eo > 0 be as in Thm. 3.1-1. Consider a family of linearly elastic flexural shells with thickness 2e, with each having the same middle surface S = 0(-~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 8(')'0) as its middle curve. Let the assumptions on the data be as above. Then, for each 0 < e < co, the scaled unknown u(e) = (ui(e)) satisfies the following s c a l e d t h r e e - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m 7~(e; f~) of a l i n e a r l y e l a s t i c f l e x u r a l shell: ~(~) e v ( ~ ) : =

{~ - (,~) e H ~ ( ~ ) ; ~ - o oil r0},

AiJkl(e)ekllZ(e; u(e))eillj(e; v ) X / ~

dx

for all v E V(~2),

where ro " - 7 0 • [-1, 1], the scaled strains eillj(e; v) are given by

e=ll~(e; v) = ~ (ae~= + oo,e) - r~~e (~),~, eall3(e;v)

-- ~

(10g o + 0o ,) -

ealla(e; V) -- e103v3,

and the functions AiJkz(e), g(e), and rPj(e) are defined as in Thin. 3.2-1. I

308

Linearly elastic flezural shells

[Ch. 6

Our main objective in this chapter consists in analyzing the behavior of the solutions u(e) E H I ( ~ ) of problems ~(e; ~) as r -+ 0. To this end, essential uses will be made of the analytical preliminaries and of the three-dimensional inequality of Korn's type for a family of linearly elastic shells (Sects. 5.2 and 5.3), already needed for the asymptotic analysis of linearly elastic generalized membrane shells carried out in the last chapter.

6.2.

CONVERGENCE DISPLACEMENTS

OF THE SCALED A S g --+ 0

We now establish the main results of this chapter: Consider a family of linearly elastic flezuval shells with thickness 2s > 0, with each having the same middle surface S = O(w) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(70) as its middle curve. Then the solutions u(s) of the associated scaled three-dimensional problems 79(s; ft) (Thin. 6.1-1) converge in Hl(f~) as s ~ 0 toward a limit u and this limit, which is independent of the transverse variable z3, can be identified with the solution ~ of a two-dimensional variational problem posed over the set w. This limit problem wiU be later identified (Thm. 6.3-1) as the scaled two-dimensional variational problem of a linearly elastic flezural shell. The functions 7a# (~/), pa#(~/), and a a~ar used in the next theorem respectively represent the covariant components of the l i n e a r i z e d c h a n g e of m e t r i c , and c h a n g e of c u r v a t u r e , t e n s o r s associated with a displacement field 71iai of the surface S and the contravariant components of the sealed t w o - d i m e n s i o n a l elasticity t e n s o r of t h e shell; we recall that e0 > 0 is defined in Thm. 3.1-1. The next result is due to Ciarlet, Lods & Miara [1996, Thm. 5.1]. T h e o r e m 6.2-1. Assume that 0 C C3(@ ~3). Consider a family of linearly elastic flezuval shells with thickness 2~ approaching zero, with each having the same middle surface S = 0(-~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(7o) as its middle curve, and let the assumptions on the data be as in Sect. 6.1.

Convergenceof the scaled displacements as e --+ 0

Sect. 6 . 2 ]

309

Let u ( e ) denote for 0 < e < so the solution of the associated scared three-dimensional problems 79(e; ~2) (Thin. 6.1-1). T h e n there exists u - (ui) E I-II(f~) satisfying u - 0 on ~o - 70 • [-1, 1] such that

U(Z) -+ u in HI(f~) as ~ -+ 0, u := (ui) is independent of the transverse variable x3. Furthermore,

-

-

~:=2

1F

i

udxa

satisfies the following s c a l e d t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b -

l e m 7>F(w) of a l i n e a r l y elastic f l e x u r a l shell: -- (~i) e V F ( 0 g ) : - - {~--(~}i) e Hl(0g) x gl(0g) x H2(0g);

7/i - 0vT/s = 0 on 70, "Yaf3(r/) = 0 in w }, 1 for all y = (~i) e VF(w), where (the definitions of the functions r~f3, ball, ~ , a af3, and a are recalled in Sect. 3.1)

~.,(~)

1 .= ~ ( o ~ .

p.,(~)

:= o . , ~ 3 - r 2 , o ~ 3

+ o.,,)

(r - r.~

- b.,~3.

- b~b~,s + b~(O,,. - r~.,~)

~b~)r/~, aa/3~r ._.-

4)V z aaf3 a~r + 2#(aa~ a [3r + aar a ~ ) ,

A+2~ pi :=

f ? fi dx3 q-h+i + hi_ a n d h ~": = h i ( 1

9, •

Linearly elastic flezural shells

310

[Ch. 6

Proof. For the sake of clarity, the proof is divided into six parts,

numbered (i) to (vi). For notational brevity, we let eillj(8 ) "-- eillj(g; U(8)) throughout the proof. (i) A priori bounds and eztraction of weakly convergent sequences: The norms

1 I~e, llj(~)lo,,and II~(e)ll~,.a~e bounded independently

of

0 < e < el, where et > 0 is given by Thm. 5.3-1. Consequently, there exists a subsequence, still denoted (u(e))e>0 for convenience, and there exist functions e illJ 1 E L 2 (f~) and u E H 1(~) satisfying u - 0 on r0 - 70 x [-1, 1] such that (recall that --+ and ~ respectively denote strong and weak convergences)" u(e) ~ u in Hl(f~) and thus u(e) --+ u in L2(f~),

1

_

1 eill j (e) ~ eillj in

L2

(~).

From the variational equations satisfied by the scaled unknown ~,(e) (Thm. 6.1-1), the asymptotic behavior of the function g(e) (Thin. 3.3-1), the uniform positive definiteness of the scaled three-dimensional elasticity tensor (Thin. 3.3-2), and the three-dimensional inequality of Korn's type for a family of linearly elastic shells (Thm. 5.3-1), we infer that

~2c-211u(~)1121,,

_ 0. Using the variational equations of the scaled variational problem 7v(e; f~) (Thm. 6.1-1) and the relations Aaf3a3(e) - Aa333(s) - 0 (Thin. 3.3-2), we may write Aijkl(~)eklll(~)eitlj(~; V ) % / f ~

+c

dx

{4A~ (~)~ll~ (~)} {~oi1~(~; *)} v/g(~i ' ~,

312

Linearly elasticflezuralshells

+ -1 ~n {Aaa'r (e)e~llr(e) + A3333(e)ealla(e)}{eealla (e;

= e2{fNfiviv/g(g)dxff-fr+uP

[Ch. 6

v)} v/g(Z) dx

hiviv/g(E)dr }.

Keep v E V(f~) fixed and let ~ ~ 0. The asymptotic behavior of the functions eeillj(s; v), the asymptotic behavior of the functions AiJkt(e) and g(e) (Thms. 3.3-1 and 3.3-2), and the weak convergences 1 1 (part (i)) together imply that: eeill/(e) ~ eillJ

{21~aa~ le~llzO3va+ (Aa

e~llr + (A + 21z)e1,13)O3v3} v/adx -- O.

Letting v vary in V(f~) then yields the other relations satisfied by 1 (if w E L 2 (f~) satisfies fu wOav dx - 0 for all v E H l(f~) the limits cilia that vanish on 70 • [-1, 1], then w = 0; cf. Thin. 3.4-1). (iv) The function U := (~i) satisfies the two-dimensional variational problem Py(w) described in the statement of the theorem. Since this problem has a unique solution (Thins. 2.6-4 and 3.3-2), the convergences u(e) -~ u in H1(~2) and u(e) -+ u in L 2 ( ~ ) (part (i)) hold in fact for the whole family (u(s))e>0 (if the function U is unique, so is the function u as it is independent of x3; el. part (ii)). Note in pass[Ie ing that reaching the same conclusion for the families -~l~J illJ(e)]e>0_ has to be postponed until part (v). That U E VF(W) has been proved in part (ii). Given art arbitrary function r / = (r/i)in the space VF(W), let the function v(e) - (vi(e)) be defined almost everywhere in f~ for all e > 0 by (the idea of constructing such a function is borrowed from Miara & Sanchez-Palencia [1996]):

va(e) := Ya - ex30a with 0a := 0ay3 + 2b~y~, v3(6) :=

First, we clearly have v(r

E V(~) for a11 e > 0,

e3[[3(8; V(8)) -- 0 for a11 e > 0.

Sect. 6.2]

313

Convergence of the scaled displacements as e -.4 0

Next, we show that, for a fized element v/E VF(w), identified wherever needed with a function in the space H t (fl) • H 1(fl) • H 2(fl), v(e) -+ 17 in Ht(~2), 1 -eallfl(e; v(e)) ---->{-xsPat3(~/)}

(~ealls(e; v(e)))

in L2(f~) as e -+ O,

converges in L2(~). e>0

The first relation clearly holds. Using the relations 7af3(v/) - 0, we find after an easy computation that

1

~o,t,~(~; ~(~)) := -7o,(~(~))~ + x~t,Slav,,(~ ) + ~bob~, v s (e) = -~s

{1

~(o~o~ + o~o~)

= -~po,(,)-

-

r.~o~

-

b;l~,7~

-

b2b~ns

}

~b;31oo,~.

Then, by Thm. 5.2-1, 1

and thus

1 -eallfl(e;

v(e)) -+ {-xspaf3(v/)}

in L2(f~).

Another computation shows that

_1 eealls (e; v(e)) = --e1 (r23(~) + b2),~ + ~rx3(~)o~ This equality, combined with the asymptotic behavior of the functions F~3(~ ) (Thm. 3.3-1) , proves that (1_ sealls(e;

v(e)) ) e>0

converges in

L2(f~). Keep the function v/C VF(w) fixed, let v - v(e) in the variational equations of problem 7~(e; f~) (Thm. 6.1-1), where v(e) - (vi(e)) is defined as supra, and let e -+ 0. The asymptotic behavior of the v(e)), the asymptotic behavior of the functions v (e) and -ei[ij(e; 1

314

Linearly elastic flezural shells

[Ch. 6

functions AiJkt(e) and g(e) (Thms. 3.3-1 and 3.3-2), the weak conver1 gences -eillJ(e) ~ ei~lj (part (i)), and the relations satisfied by the c

t (part (iii))together yield limits eill3

lim 1 fn A~Jkl

{/o

= e-~olim Aa~r(s){~ +

/~A~

+ +

1~

---- --

1

1 eotJ,(~; ~)}V~(~)d~

4a~

/a

+ = -~

1 lit(S)} v/g(e) dx ,,)}4g(~)d~

1 A ~ ( ~ ) { ~11,(~)} 4g(~l d~ A~(~){~II~(~)}{~ -~11~(~; ~)} v / g ~ d~

~3

aa~O'r 1

~ll~,~(,7)v~d~

x3 ,~+ 2#

+ "(ha~ a'r +

) ecrllrpa/3(W)~dx

= e--+O lim {fa 'ivi(e)V/'g(e)d:r+fr + u r _ hivi(e)v/g(e)dF} : s =

+ ~ S~a~ + h~ + h' ~v~dy.

We have yet to take into account the relations pa/3(u) - -03e~ll ~.~ in L2(~) (part (iii)). Since the function u is independent of x3 (see i are of the form part (ii)), these relations show that the functions ea"~llp 1

%11~3- Ta~ - x3pa/3(U) with T ~ c L2(w).

Sect. 6.2]

Convergence of the scaled displacements as e --+ 0

315

Therefore

2

x3a

% l l r P a ~ ( r l ) ~ dx -- -~

"~3"*

= -~

t,~r(U)pa/3(rl)V/-d d=

a a~'rp~r(~)pa~(rl)V~ dy,

and thus we have established that the variational equations of problem 79F(w) are satisfied by ~. (v) The weak convergences -eillj(s 1 : ) ~ eillJ in L2 (f~) established

in part (i) are in fact strong: :

1

~eillJ(S ) -+ eillJ in

L2

(a).

Besides, the Kmits e~ltJ are unique; hence these convergences hold for / \ 1 the whole family , r /(-eilJ(e)}e> O. Combining the uniform positive definiteness of the scaled elasticity tensor and the asymptotic behavior of the function g(s) (Thms. 3.3-1 and 3.3-2) with the variational equations of problem 7~(e; [2) where we let v - u(e), we obtain

c : : go:/2 ~

i,j

1

I~,llj(~)

-

: 2 ~lljlo,~

1

1

< A(s) -

--,

where n

1

z

= f~/~,(~)v/g(~) ~+ f~+ur_ h~,(~)v/g(~)dr -

AiJkl(e){eekllZ(e )_ -

z ~klj~

1 v/g( } ~,llJ

~1

e~.

The asymptotic behavior of the functions A#m(e) and g(s) together with the convergences ui(s) --+ ui in L2(f~) and ui(e) ~ ui in Hl(f~) (the latter implying that tr ui(e) -~ tr ui in L2(r+ u r _ ) ) and

316

[Ch. 6

Linearly elastic flezural shells

1 1 the weak convergences ~eillJ(e ) --~ eillj

i n L 2 (if2)

A := l i m A ( e ) - f y ' u , ~ d ~ + f ~ e--+O

(part (i))imply that

+ur_

hiuivZddF

- f. Using the expressions of the functions A~Jk~(0) (Thm. 3.3-2) and eill s l (part (iii)) and recalling that u - (ui) is independent of xa (part (ii)), we next infer that A "-

fi

dxa + h i+ + h i-

1

}

Ui %/c~dy

- ~1

/o

dafter %llreallf3 1 1 ~

dx.

The relations pail(u) - -03elallfl in L2(~) (part (iii)) imply that eallf~l -- T a r 1 - X 3 P a f l ( ~ ) with Taf~ E L2(w); hence

1

a afl~re~llreallflV/-d dx - 2

f

+ -~

T ~ r T a f 3 ~ dy a afl~rpar(u)pafl(-u)V~ dy.

Since ~ satisfies the variational equations of problem 79F(w) (see part (iv)), we thus have A = - f~ aa/3~r T~r T aft V~ dy.

Noting that A > 0 (the numbers A(s) are >_ 0 by their definitions) and that the scaled two-dimensional elasticity tensor of the shell is uniformly positive definite in ~ (Thm. 3.3-2), we conclude that Taft - 0. These relations have two consequences" First,

1 1 hold in L 2( ~ ) . and thus the strong convergences ~eillj(e ) --+ eillj Second, the functions e ~11/3 1 are uniquely determined, since they are given by and the function ~ is unique (part (iv)). That the functions e/113 are uniquely determined then follows from the relations established in part (iii).

Sect. 6.3]

317

The two-dimensional equations

(vi) The weak convergence u(~) part (i) is in fact strong: u(e) ~ u in

u

in

H~(~)

established in

H~(n).

By Thm. 5.2-2, it remains to show that each family (paf3(u(e)))e>o strongly converges in H - i (~). Since -~eall~(e 1 i 3 in L 2(12) by ) -4 eallf part (v), we first have

103eallf3(g ) ~ 03elllfj in H-I(~'~). By Thm. 5.2-1, we next have 1

-~ 0 in H - i ( n ) .

Hence

--03eall~} in H and the proof is complete.

6.3.

m

THE TWO-DIMENSIONAL EQUATIONS OF A LINEARLY ELASTIC FLEXURAL SHELL; EXISTENCE AND UNIQUENESS OF SOLUTIONS

The next theorem recapitulates the definition and assembles the main features of the limit two-dimensional problem 7~F(w) found at the outcome of the asymptotic analysis carried out in Thm. 6.2-1. The existence and uniqueness theory, which is quickly reviewed in this theorem, is expounded in detail in Sect. 2.6, where ad hoc references are also provided. T h e o r e m 6.3-1. Let w be a domain in I~2, let 7o be a subset of the boundary of w with length Vo > 0, and let 0 E C3(~; R 3) be an injective mapping such that the two vectors aa - OaO are linearly

318

Linearly elastic flezural shells

[Ch. 6

independent at all points of-~ and such that V~(w) # {0}, where

VF(~)

(,i) e m(~) • HI(~) • H~(~);

'-- { ~ -

~i "-- 0t, r/3 -- 0 011 ")'0, "Ycq3(l?) -- 0 ill OJ},

1

The associated scaled two-dimensional variational p r o b l e m 79F(w) of a linearly elastic flexural shell: Given pi E L 2 ( w ) , find = (~i) that satisfies

r c vF(w), 1

for all r / = (r/i) 6 VF(w),

where p~,(,)

.= o~~

- r~,o~

+b~(O~,

aa/3~r .__

-

- b~b~,~3 + b ~ ( O , ~

r~,~) +

(Oob~ + r ~ b 3

-

r~,)

~b~).~, ~

- r~

4A# aa~a~r + 2# (a a~a[3r + aaragl~), A+2p

has one and only one solution, which is also the unique solution of the minimization problem: Find ~ such that e Vv(w) and j v ( ~ ) = iF(n) := g

inf

iF(Y), where

/.

p~,(n)pa/9(n)~dy- p'yix/-ady.

Proof. The existence and uniqueness of a solution to the variational problem :PF(w), or to its equivalent minimization problem, is a consequence of the inequality of Korn's type on a general surface (Thin. 2.6-4), of the uniform positive definiteness of the scaled

Sect. 6.3]

The two-dimensional equations

319

two-dimensional elasticity tensor of the shell (Thm. 3.3-2), of the inequalities a(y) > a0 > 0 for all y C ~ (Thin. 3.3-1), and of the Lax-Milgram lemma, m The minimization problem encountered in Thm. 6.3-1 (or that in Thm. 6.3-2 below in its "de-scaled" formulation) provides an interesting example of a minimization problem with "equality constraints", namely the relations "Vaf3(v/) = 0 in w" that the elements v/of the space over which the functional is to be minimized must satisfy. Normally, a Lagrange multiplier is then attached to such a problem (see, e.g., Ciarlet [1982, Thm. 7.2-2]), allowing in turn to write the boundary value problem that is (at least formally) equivalent to the minimization problem; this is the case for instance of the limit "multi-dimensional" equations found at the outcome of the asymptotic analysis of elastic multi-structures (see Vol. II, Chap. 2; especially Sect. 2.5). Finding the Lagrange multiplier in the present case seems more challenging. In this direction, see Sanchez-Hubert ~5 Sanchez-Palencia [1997, Chap. 8], Brezzi, G~rard & Sanchez-Palencia [1998], Sanchez-Valencia [1999]. In order to get physically meaningful formulas, it remains to "descale" the unknowns ~i that satisfy the limit scaled problem 7~F(w) found in Thm. 6.2-1. In view of the scalings

u~(e)(x) - u~(x ~) for all x ~ : 7rex e ~ made on the covariant components of the displacement field (Sect. 6.1), we are naturally led to defining for each e > 0 the eovaria n t c o m p o n e n t s ~ 9~ -+ I~ of the limit d i s p l a c e m e n t field 9 w --+ of the middle surface S of the shell by letting (the vectors a i form the contravariant basis at each point of S)

~'~ "- ~'i and ~e := ~.~ai" A w o r d of c a u t i o n . Like those found in the analysis of linearly elastic elliptic membrane shells (Sect. 4.5), the fields ~ := ( ~ ) and ~e = ~ a i must be carefully distinguished! The former is essentially a convenient mathematical "intermediary", but only the latter has physical significance. II

Linearly elastic flezural shells

320

[Ch. 6

Remark. Conceivably, the limit scaled displacement field across the thickness of the shell could also be de-scaled, resulting into a limit displacement field ire(O) 9-~e --+ ~3 inside the shell defined by (the vectors 9i, e form the contravariant basis at each point of the reference configuration O(~e); cf. Sect. 3.1)" .:

',*,

since the scaled limit u = (ui) is independent of the transverse variable x3 (Thin. 6.2-1). For the same reason, however, the de-scaled field does not inherit any remarkable structure as x~ varies across the thickness of the shell. By contrast, the limit displacement field across a plate, which is a linearly elastic flexural shell (Ex. 6.3), is a Kirchhoff-Love one (Vol. IX, Thm. 1.7-1). However, it does inherit this richer structure only because different scalings can be made in this case on the "horizontal" and "vertical" components of the displacement field. II Recall that fi, e C L2(n e) and h i'e C L2(r~_ kJ re_) represent the contravariant components of the applied body and surface forces actually acting on the shell and that Ae and #e denote the actual Lam6 constants of its constituting material. We then have the following immediate corollary to Thms. 6.2-1 and 6.3-1; naturally, the ezisfence and uniqueness results of Thm. 6.3-1 apply verbatim to problem 7~(w) (for this reason, they are not reproduced here)" T h e o r e m 6.3-2. Let the assumptions on the data and the definitions of the functions 7a~(r/) and Pa~(~7) be as in Tam. 6.2-1. Then the vector field ~e := (i~) formed by the covariant components of the limit displacement field ~ a i of the middle surface S satisfies the following t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m 7~(w) of a l i n e a r l y elastic f l e x u r a l shell:

~e E V F ( w ) : = {~/= (~i) E Hi(w) • Hi(w) • H2(w); ~i -- 0u~3 = 0 on 70, 3'ag~(r/) = 0 in w},

V

ePzr(~e)Pa;3(~l)v~dY =

P"e~lix~dY

=u n = (w) e

Sect. 6.3]

The two-dimensional equations

321

where a a ~ , ~ ._.-- 41he#e aa~a~r + 2#e(aa~a~r + aaraDCr), ,V + 2# e pi,~ : :

f,,E dx~ + h ; e + h ''e and h~ e "- h i'e(., :kr f~

E

"

~

~

.

Equivalently, the field ~ -- (i~) satisfies the following minimization problem: ~ e VF(w)

and j ~ ( ~ e ) _

inf j~(r/), where ncvF(~)

II Each one of the two formulations found in T h m . 6.3-2 constitutes the t w o - d i m e n s i o n a l e q u a t i o n s o f a l i n e a r l y e l a s t i c f l e x u r a l shell. We recall that the condition V e ( w ) # {0), which is the basis of the definition of a linearly elastic flexural shell, means that there exist nonzero a d m i s s i b l e l i n e a r i z e d i n e x t e n s i o n a l d i s p l a c e m e n t s of the middle surface (Sect. 6.1), since the functions "yaf3(r/) used in the definition of VF(w) are the covariant components of the l i n e a r i z e d c h a n g e o f m e t r i c t e n s o r associated with a displacement field yia i of the middle surface S. In order to interpret the boundary conditions ~ - Ov~ on ")'0 satisfied by the field ~e - ( ~ ) , let rlia i be a displacement field of the middle surface S - 8(~) with smooth enough, but otherwise arbitrary, covariant components r/i 9~ --+ R. The tangent plane at an a r b i t r a r y point O(y) + yi(y)ai(y), y E -~, of the deformed surface (O + rlia*)(-~) is thus spanned by the vectors o.(o +

- a.(y) +

+

if these are linearly independent. Since ~i - 0 ~ 3 - 0 on 70 ~

~i - O~r/3 - 0 on 70,

Linearly elastic flezural shells

322

[Ch. 6

it follows that

O(y) + 71i(y)ai(y) - O(y) for aU y e 70, Oa(O + z}iai)(y) - aa(y) + Oaz}/3(y)af3(y) for all y C 70. These relations thus show that the points of the deformed and unde[ormed middle surfaces, and their tangent spaces at those points where the vectors Oa(O+~Iia i) are linearly independent, coincide along the set 0(7o). Such t w o - d i m e n s i o n a l b o u n d a r y c o n d i t i o n s of c l a m p i n g are suggested in Figs. 6.1-1 to 6.1-3. The functions Pa/3(W) are the covariant components of the line a r i z e d c h a n g e of c u r v a t u r e t e n s o r associated with a displacement field 7}iai of the middle surface S and the functions a afJav, e are the contravariant components of the t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of t h e sheU, already encountered in the two-dimensional equations of linearly elastic elliptic membrane and generalized membrane sheUs (Thins. 4.5-2 and 5.7-2). FinaUy, the functional j~ 9VF(w) -+ IR is the t w o - d i m e n s i o n a l e n e r g y , and the functional

is the two-dimensional strain energy, of a linearly elastic flexural shell. Note that the s a m e two-dimensional problem 7)~(w) is evidently obtained if the scalings on the unknowns are the same as before, i.e., ~ ( x ~) - u i ( ~ ) ( x ) for aU x e - ~ex E ~~,

but the following more general a s s u m p t i o n s on t h e d a t a are made:

Ae = etA _

and all

#e = et#, -

n

where the constants A > 0 and # > 0 and the functions fi C L2(~) and h i E L2(p+ U r _ ) are independent of e and t is an arbitrary real

Sect. 6.4]

Justification of the two-dimensional equations

323

number. Besides, the analysis of Sect. 3.4 shows that these assumptions on the data are the only ones possible for flexural shells. Remark. A different kind of generalization is possible. For definiteness, assume that the Lamd constants are independent of e. Then it is easily verified that the same scaled limit problem 7~F(w) is obtained under the assumptions that

fi, e(Xe ) _

e2fi(~; :g) for

all z e - 7r~z e f~e,

h~"(~ ~) = ?h~(~; ~) fo~ ~11 ~" - ~ ' ~ c r ~ u r'_, and

fi(e; .) ~ f i in L2(~2) as e --+ 0, hi(s; .) -+ h i in L2(r+ u r _ ) as s ~ 0. The functions p~ appearing in the right-hand sides of problem 7~(w) are then defined by

fi dx3 + h i+ + h i_~. 1

)

B

6.4.

JUSTIFICATION OF THE TWO-DIMENSIONAL EQUATIONS OF A LINEARLY ELASTIC FLEXURAL SHELL; COMMENTARY AND REFINEMENTS

It remains to convert in terms of de-scaled unknowns the fundamental convergence theorem established in Sect. 6.2. As the "originaP' unknowns u ie are defined over a domain that varies with e (the set ~t~) , their averages -~ f_~ u ie dx~ are more appropriate for this purpose, since they are defined over a fixed domain (the set w). The convergences ui(e) --+ ui in H I ( ~ ) (Thm. 6.2-1), the scalings ui(~)(x) - u~(x ~) for all x ~ - 7r~x e ~e (Sect. 6.1), the de-scalings

~ - ~i - 89fl_ 1 ui dx3 (Sect. 6.3) and Thm. 4.2-1 together yield the following convergences of the averages 2~ f-~ u~ dx~ of the covariant components of the "original" three-dimensional displacement:

1 F e~

2e

d:~ -~ r i~ H~(~).

Linearly elastic flezural shells

324

[Ch. 6

However, these convergences can be further improved and given a more intrinsic character by considering instead the averages of the tangential component Ueaona'e and of the normal component u~g 3,~ of the three-dimensional displacement vector itself; note in this respect that, along a given normal direction to the surface S, the vectors ga, e and g3, 9remain respectively parallel to the tangent plane and normal e ~ g3, e - a3, and gie " g~'" e : Ji" j More to S since gea - a a - x3baacr, specifically, the above convergences combined with the behavior as e --+ 0 of the vectors gi, e lead to the following result: 6.4-1. Assume that B E C3(~; I~3). Consider a family of linearly elastic flexural shells with thickness 2e approaching zero, with each having the same middle surface S - 8(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(70) as its middle curve, and let the assumptions on the data be as in Sect. 6.1. Theorem

Let (u~) e H I ( ~ ~) and (i~) e H i ( w ) • H i ( w ) x H2(w) respectively denote for each e > 0 the solutions to the three-dimensional and twodimensional problems 7~(~ e) and 7~(w) (Sect. 3.1 and T a m . 4.6-1). Finally, let (ii) e H i ( w ) • H i ( w ) • denote the solution to problem T'e(w) (Thin. 6.3-1), which is thus independent of Th~

e a ~ae - Ca and thus Caa

~aa a in H 1(w) for all e > 0,

Hl( o)

--

2e

e a,,

o,

and

- ~3 and thus ~ a 3 -

~3a3 in H2(w) for all e > 0,

lf_ ~u~g 3'~ dx~

3 in H i ( w ) a s e ~ 0.

2e

~ r

e

Pro@ The proof is similar to that of T h m . 4.6-1. The assumption 8 E C3(~; I~3) implies that the vector fields ga(e) . ~ _+ IR3 defined by ga(e)(x):-" ga'e(xe) for all x e - r e x e ~e are such t h a t

Sect. 6.4]

Justification of the two-dimensional equations

325

g~(e) - a a - O(e) in CI(~). Since

2r

u~g a'~ dz~ - ~ a a = -

2

i

u ~ ( ~ ) ( g ~ ( ~ ) - a ~) a~3 - ( , , ~ ( ~ ) - r

the convergences ua (r imply that

~,

--+ ua in H I (12) and ga(e) ~ a a in Ci (~)

=~(~) ( a ~ ( ~ )

- a ~) -~ 0 in H ~ ( a ) ;

hence 1 fl_l u,~(e)(g,~(e)_ a a) dz3 --4 0 in HI(w) by Thin. 4.2-1. The same theorem also shows that (ua(e) - ( a ) a a --+ 0 in Hi(w). Since 2

2s

,,~g3,~ a ~

- C~,~ ~ - (,,3(~) - 6 ) a ~

e

the same theorem shows that ( u 3 ( e ) - ~z)a 3 --+ 0 in I-Ii(~).

II

-e _ --+ R 3 and ~N -~ _ --4 R 3 defined by The fields ~T "w "w

:= ~aa

and ~N := ~ a3'

which appear in Thm. 4.6-1, are respectively called the l i m i t t a n g e n t i a l d i s p l a c e m e n t field and the limit n o r m a l d i s p l a c e m e n t field of the middle surface S of the shell. Naturally, they are related to the limit displacement field ~e _ ~ a i of S (Sect. 6.3) by

Under the essential assumptions that the space VF(w) contains nonzero elements, we have therefore justified by a convergence result (Thm. 6.4-1) the two-dimensional equations of a linearly elastic flezural shell. In so doing, we have justified the formal asymptotic approach of Sanchez-Palencia [1990] (see also Miara & Sanchez-Palencia [1996] and Caillerie & Sanchez-Palencia [19955]) when "bending is not inhibited", according to the terminology of E. Sanchez-Palencia. Credit should be given in this respect to Sanchez-Palencia [1989a] for recognizing the central r61e played by the space VF(w) in the classification of linearly elastic shells.

326

Linearly elastic flezural shells

[Ch. 6

A w o r d of c a u t i o n . In a flexural shell, body forces of order O(e 2) thus produce an O(1) limit displacement field. By contrast, body forces of order O(1) are required to also produce O(1) limit displacement fields in an elliptic membrane shell. Both types of shells thus exhibit strikingly different limit behaviors! This conclusion of a mechanical nature simply reflects that strikingly different three-dimensional inequalities of Korn's type (compare Thm. 4.3-1 with Thm. 5.3-1) are needed for deriving in each case the fundamental a priori bounds in the convergence theorems (compare parts (i) of the proofs of Thms. 4.4-1 and 6.2-1). II After the original work of Ciarlet, Lods & Miara [1996] described in this chapter, the asymptotic analysis of linearly elastic flexural shells underwent several refinements and generalizations: First, Genevey [1999] has shown that the convergence result of Thm. 6.2-1 can be also obtained by resorting to P-convergence theory. Other useful extensions include the justification by an asymptotic analysis of linearly elastic flezural shells with variable thickness (Busse [1998]; see Ex. 6.7) or made with a nonhomogeneous and anisotropic material (Giroud [1998]), the convergence of the (scaled) stresses and the explicit forms of the limit stresses (Collard & Miara [1999]; see Ex. 6.8), an asymptotic analysis of the associated eigenvalue problem (Kesavan & Sabu [1999a]) and time-dependent problem (Xiao Li-ming [1999a]). The surprising phenomena appearing when a linearly elastic flexural shell "becomes a plate" are investigated in Ciarlet [1992a, 1992b], Sanchez-Palencia [1994], and Lods [1996]. An asymptotic analysis similar in its principles can be applied to linearly elastic curved rods, whose limit behavior is always "flexurar'; see Alvarez-Dios & Viafio [1997], Jamal [1998]. We conclude this commentary by examining linearly elastic plates, which constitute examples of linearly elastic flexural shells (as already observed; cf. Fig. 6.1-3), since

v F ( ~ ) - { ~ - (0, o, ~3); ~3 e H~(~); ~3 - 0~3 - 0 o . ~0} ~ {0} in this case; naturally, we assume that the mapping 0 is of the form O(y~, y2) = (y~, y~, o) for an (ys, y2) ~ ~. Assume that there exist constants A > 0 and # > 0 and functions f i e L2(~) and h i E L2(r+ u r_) independent of ~ such that, for

Justification of the two-dimensional equations

Sect. 6.4]

327

each e > 0, the Lam6 constants )~e a n d tte of the m a t e r i a l constit u t i n g the plates a n d the Cartesian components j::,e . ~t~ __+ ]R a n d h/,e 9F~_ U F ~_ -+ I~ of the applied b o d y a n d surface forces (the set ~e is now the reference configuration) satisfy o

)~e = )~

and

#e = #,

_ ~2/~(~)

fo~ an

~ - .~

z n~,

h~,~ ( ~ ) _ ~3 h~(~)

fo~ all

~ - .~

~ r ~ u r~_,

/~,~(~)

a n d let the scaled u n k n o w n u ( s ) - (ui(s)) e Hl(~t) be defined by

ui(s)(z) := u~(z e) for all z ~ - 7rex e ~e. where the functions u i -+ It~ are the Cartesian c o m p o n e n t s of the displacement field of the plate. T h e n T h m . 6.2-1 shows that, in this case, there exists a function U3 E H2(~t) vanishing on F0 - 7 0 • [ - 1 , 1] such t h a t

u(e) - (ui(e)) -+ (0, O, u3) in I-I~(~2) as ~ -+ 0, u3 is i n d e p e n d e n t of the transverse variable x3,

~3 "-- ~

I U3 dz3 ~ V3(w),

1- ~ ba~avO~T~3Oa3rl3dy= fwp3rl3 dy for all rl3 ~ V3(w)

3 where

b~

~. .-.- 4 ~ ~~. A+2/z

+ 2~(6~~.

+ 6~.6~),

p3 :._ l_ f dx 3 + (h3+ + h 3_) and h 3, :-- h 3(., --~-1). 1 However, this result is only a special case of the "classical" convergence t h e o r e m for a plate; see Vol. II, Thin. 1.4-1. For, w h e n the a s y m p t o t i c analysis is applied in ibid. to a linearly elastic plate,

more freedom is allowed, as regards both the choice of scalings of the displacement field and the choice of the asymptotic assumptions on the applied forces. More specifically, another scaled u n k n o w n ~(~) = (~2i(e)) is defined in this case by letting ~(~)(z)

- su~(z ~) a n d ~3(s)(z) - u~(z ~) for all z ~ e ~ ,

328

Linearly elastic flezural shells

[Ch. 6

and the applied forces are such that there exist functions ]i E L2(fl) and h / E L2(F+ U F_) independent of e such that fa'e(X~) -- e]~(X) and ]3'e(xe) ha'e(x e)

-

-

e2/3(X) for all m E ~,

g2ha(x) and h3,e(x ~) - e3h3(x) for all x e r + [J r _ .

The cruder scalings and assumptions made when the plate is considered as a special case of a shell have two consequences: First, the horizontal components fa, e and h a'e of the applied forces do not contribute to the definition of the limit two-dimensional problem satisfied by the unknown ~3. Second, the de-scaled components of the limit displacement field (0, 0, ~3) found in this fashion are all of order zero with respect to s. Therefore, the de-scaled horizontal components of the limit displacement field that are of order one with respect to s are necessarily "ignored" in this approach. These horizontal components, together with the transverse component of order zero, form a KirchhofJ-Love displacement field (Vol. II, Thm. 1.7-1) inside the plate. Another major difference is that the asymptotic analysis of a linearly elastic plate yields a limit problem that simultaneously includes flexural and membrane equations. The reason why limit membrane equations are in addition obtained is again that horizontal components of order one of the limit displacement field can be recovered, thanks again to the refined scalings and assumptions that are allowed for a plate. That cruder scalings and assumptions are unavoidable for "genuine" shells has been rigorously established in Sect. 3.4, after Micra & Sanchez-Palencia [1996].

EXERCISES

6.1. Let f = (fa) E C2([0, 1]; IR2) be an injective mapping such that f ' ( t ) # 0 for all t E [0, 1] and let S - 8(~), where w --]0, 1[• 1[ and 8(t, z) - fa(t)e a + ze 3 for (t, z) E ~. The surface S is thus a portion of a cylinder orthogonal to, and passing through, the planar curve f([0, 1]); cf. Fig. 6.1-1.

Ezercises

329

(1) Assume that

0'o C {(O,z) CI~2; O_ 0 the contravariant components of the linearized stress tensor field (Thm. 1.6-1) inside each shell and define the scaled stresses a '3 (e) 9f~ --+ R by letting . o

~iJ'~(x~) --: aiJ(~)(x) for all x ~ - 7r~x e ~. Note that the scaled stresses then satisfy

criJ(s) - AiJkl(s)eklll(S; u(s)). Show that l a a ~ (e) _+ aa~, 1 in L2(f/),

~

o'i3(e) --~ cri3'2 in H i ( - 1 , 1; H - l ( w ) )

332

Linearly elastic flezural shells

[Ch. 6

as ~ --+ 0, where the limits are given by (covariant derivatives na#[~ are defined in Thm. 4.5-1)

aa~, 1 _ _x:3aaf3ar par(u), aaa, 2 = 1 ( x 2 _ 1)(aaf3~rO~r(g))l~ , 2 aaa, 2 _ l(x~ - 1)a a ~ r

Remark. These results should be profitably compared with those established for linearly elastic membrane shells (Ex. 4.4) and plates (Vol. II, Sect. 1.6).

CHAPTER 7 KOITER'S

EQUATIONS

TWO-DIMENSIONAL

AND

LINEAR

OTHER

SHELL THEORIES

INTRODUCTION

Consider as in the previous chapters a linearly elastic shell with middle surface S - 8(~) and thickness 2e, subjected to a boundary condition of place along a portion of its lateral face with 8(70) as its middle curve, and subjected to applied forces. This problem can thus be modeled either by the equations of threedimensional linearized elasticity (Chap. 1) or by two-dimensional equations obtained by an asymptotic analysis of the three-dimensional equations. We showed that the form of these two-dimensional equations depends on, and only on, the geometry of the surface S and on the set ~'0 (Chaps. 4 to 6). Founding his approach on a priori assumptions of a geometrical and mechanical nature about the solution of the three-dimensional equations (these assumptions are described in Sect. 7.1), W.T. Koiter has devised in the sixties yet another means of modeling the same problem by two-dimensional equations. The resulting two-dimensional Koiter equations for a linearly elastic shell take the following form, when they are expressed as a vari~ho~ r a~e ational p~obl~m: The unknown r - (r the covariant components ~:,i " ~ --+ I~ of the displacement field ~ : , i a ~ of the points of the middle surface S, satisfies: o

(~: - ( ( g , i )

E Vg(w)-

{n-

(Yi) E Hi(w) • Hi(w) • H2(w); ~i = 0~3 = 0 on 70},

g3

/~p~'~n~vqdy

for ~H n - (n~) E V ~ ( ~ ) ,

where

a a13~r'e a r e

the components of the two-dimensional elasticity

334

Koiter's equations and other linear shell theories

[Ch. 7

tensor of the shell, 7 ~ ( ~ ) and Pal3(r/) are the components of the linearized change of metric and change of curvature tensors associated with a displacement field ~Tiai of S, and the given functions pi, e E L2(w) account for the applied forces. Equivalently, the unknown ~ satisfies the following minimization problem: ~

E VK(W) and j ~ ( ~ )

=

inf j~(v/), uev~(~)

where the two-dimensional Koiter energy j ~ 9VK(W) --+ R is defined by j EK( n ) = -~

{ s a a~ar' eVar (17) Vaf3( n ) S3 aa[3trr, +-~-

~

~

"

As already shown in Sect. 2.6, the existence and uniqueness of a solution to these equations essentially rely on an inequality of Korn's type on a general surface, itself a consequence of a crucial lemma of J.L. Lions and of an infinitesimal rigid displacement lemma on a general surface; this existence and uniqueness result is recalled in Sect. 7.1, together with its extension to shells whose middle surface has "little regularity" (Thms. 7.1-1 and 7.1-2). In addition, we identify the associated boundary value problem and we give sufficient conditions for the regularity of its solution (Thm. 7.1-3). It is remarkable that Koiter's equations can be fully justified for all types of shells, even though it is clear that these equations cannot be recovered as the outcome of an asymptotic analysis of the threedimensional equations, since Chaps. 4 to 6 exhaust all such possible outcomes! More specifically, we show that, for each category of linearly elastic shells (elliptic membrane, generalized membrane, or flexural), the 1 fields ~eg and 2ss

f2

e u e dx~, where u e denotes the three-dimensional

solution, have the same asymptotic behavior in ad hoc functional spaces as ~ --+ 0 (Thms. 7.2-1 to 7.2-3). So, even though Koiter's linear model is not a limit model, it is in a sense the "best" two-dimensional one for linearly elastic shells ! One can thus only marvel at the insight that led W.T. Koiter to conceive the "right" equations, whose versatility is indeed remark-

Sect. 7.1]

The two-dimensional Koiter equations

335

able (see the commentary in Sect. 7.3), out of purely mechanical and geometrical intuitions! While Koiter's equations belong to the family of Kirchhoff-Love theories (Sect. 7.1), two-dimensional shell equations that rely on the notion of one-director Cosserat surfaces have also been proposed by P.M. Naghdi, again in the sixties. After describing the associated twodimensional Naghdi equations for a linearly elastic shell (Sect. 7.4), we review the existence and uniqueness theory for these equations, which is akin to that for Koiter's equations (Thm. 7.4-1). Finally, we briefly review in Sects. 7.5 and 7.6 other two-dimensional equations that have also been proposed for modeling linearly elastic shells, notably "shallow" shells.

7.1.

THE TWO-DIMENSIONAL KOITER EQUATIONS F O R A L I N E A R L Y E L A S T I C SHELL: EXISTENCE~ UNIQUENESS, AND REGULARITY OF S O L U T I O N S ; F O R M U L A T I O N AS A BOUNDARY VALUE PROBLEM

Let w be a domain in I~2 with boundary "y, let O C Cs(~; I~s) be an injective mapping such that the two vectors aa = OaO are linearly independent at all points of ~, and let ~0 be a portion of "y that satisfies length ~/o > O. Consider as in the previous chapters a linearly elastic shell with middle surface S = O(~) and thickness 2s > 0, i.e., a linearly elastic body whose reference configuration is the set O(~e), where : =

o(y,

-

0(y) +

(y,

e

The material constituting the shell is homogeneous and isotropic and the reference configuration is a natural state, so that the material is characterized by its two Lamd constants )~e > 0 and #e > 0. The shell is subjected to a boundary condition of place along the portion o ( r ~ ) of its lateral face, where r~ . - -y0 • [-e, e], i.e., the three-dimensional displacement vanishes on | Finally, the shell is subjected to applied body forces in its interior | and to applied surface forces

Koiter's equations and other linear shell theories

336

[Ch. 7

on its "upper" and "lower" faces and | ~_), their densities being given by their contravariant components ]i,e C L2(f~ e) and h

e

u

where

-



In a seminal work on shells, John [1965, 1971] has shown that, if the thickness is small enough, the state of stress is "approximately" planar and the stresses parallel to the middle surface vary "approximately linearly" across the thickness, at least "away from the lateral face". In Koiter's approach (Koiter [1960, 1966, 1970]), these approximations are taken as an a priori assumption of a mechanical nature (a precise statement of this assumption is found in Sect. 11.1) and combined with another a priori assumption of a geometrical nature, called the Kirchhoff-Love assumption: Any point on a normal to the middle surface remains on the normal to the deformed middle surface after the deformation has taken place and the distance between such a point and the middle surface remains constant (Ex. 7.1(1)). In fact, this assumption is required to hold only "to within the first order" in the linearized theory considered in this chapter, in which case it is called the linearized Kirchhoff-Love assumption (Ex. 7.1(2)).

Remark. In a pioneering contribution, Oden, Wempner &: Kross [1968] have suggested to incorporate some discretized version of the linearized Kirchhoff-Love assumption into finite element codes, typically by requiring that it be only satisfied on a finite set of points. In myriad numerical simulations, this idea has since then proved to be highly judicious, m Taking these two a priori assumptions into account, W.T. Koiter then shows that the displacement field across the thickness of the shell can be completely determined from the sole knowledge of the displacement field of the points of the middle surface S, and he identifies the two-dimensional problem, i.e., posed over the two-dimensional set ~, that this displacement field should satisfy. As in the two-dimensional theories encountered so far, the unknown is a vector field, now denoted ~ : -- (~ie,g ) 9 ~ ~ ]~3, whose components iie, g " "~ --~ I~ are the covariant components of the displacement field of the middle surface S. This means that ii~,g(y)ai(y) is the displacement of the point 0(y); cf. Fig. 7.1-1. In their linearized version (the nonlinear one is given in Sect. 11.1), the equations found by W.T. Koiter consist in solving the following

The two-dimensional Koiter equations

Sect. 7.1]

337

F

Fig. 7.1-1: A linearly elastic shell modeled by Koiter's two-dimensional equations. T h e t h r e e u n k n o w n s are the covariant c o m p o n e n t s (i~,/c : w --+ IR of the displacem e n t field of t h e m i d d l e surface S; this m e a n s t h a t (ie,lc(y)ai(y) is t h e displacem e n t of t h e p o i n t O(y) of the middle surface S. T h e " two-dimensional b o u n d a r y c conditions of clamping" (i,9~c = 0 ~(s,/r = 0 on 70 m e a n t h a t the points of, a n d the t a n g e n t spaces to, the deformed and u n d e f o r m e d middle surfaces coincide along the set 0('1,0).

variational problem 7>~c(W)(the associated boundary value problem is given in Thm. 7.1-3)" Find ~ c - ((~c,i) such that

77i - 0~77~ -

0 on

70

},

= f pi'enix~dy for all r l - (rli) E V g ( w ) , d~

338

[Ch. 7

Koiter's equations and other linear shell theories

where (the functions a a~3, ba~3, b~, see, e.g., Sect. 3.1): a ~ , ~ ._ 9-

4Aepe A~ + 2# e

r:,,

and a are defined as usual;

a ~ a ~ + 2#~(a~a~ + a ~ a ~ )

1

po,(v) :=

oo, w -

- b~b~73

a~

+b~(O~w - r ; , w )

+(oob; + rLb pi , . _

2

+ b;(O~w - rLw

)

-

]i "da:~ + .0+ + h"

and h'_t'e "- h"e( ., +s).

e

The functions 7a# (r/) and pa#(r/) are the customary covariant components of the linearized c h a n g e of m e t r i c and c h a n g e of c u r v a t u r e t e n s o r s associated with a displacement field y i a i of the middle surface S and the functions a a/3~r,e are the customary contravariant components of the t w o - d i m e n s i o n a l elasticity t e n s o r of t h e shell. Note that Destuynder [1985] has found an illuminating way of deriving the same linear Koiter equations from three-dimensional elasticity, which uses a priori assumptions only of a geometrical nature. 1

The ezistence and uniqueness of a solution to problem T'~:(w), which essentially follow from the Vg(w)-ellipticity of the bilinear form, was first established by Bernadou & Ciarlet [1976]; a more natural proof was subsequently proposed by Ciarlet & Miara [1992b], then combined with the first one in Bernadou, Ciarlet & Miara [1994]. This proof, which has been already given and discussed at length in Sect. 2.6, is simply outlined in the next theorem. Observe that 0 C Ca (~; IR3) is precisely the assumption that will afford the justification of Koiter's equations in Sect. 7.2. T h e o r e m 7.1-1. Let w be a d o m a i n in I~2, let 70 be a subset of 7 - Ow with length 70 > 0, and let 0 E C3(~; ~3) be an injective m a p p i n g such that the two vectors an = OaO are linearly i n d e p e n d e n t at all points of -~.

Sect. 7.1]

339

The two-dimensional Koiter equations

Then the variational problem 79~(w) has one and only one solution, which is also the unique solution to the minimization problem: Find ~K -- ( ~ , i ) such that r

C Vg(w) and J~c(r

-

inf j~(rl), where ,ev~(~)

1 e 3 aa/3ar'

pi' e~Ti~ dy.

Proof. The assumptions fi, e C L2(~2~) and h i'~ C L2(r u r t ) imply that pi,~ C L2(w). The existence and uniqueness of a solution to the variational problem :P~:(w), or to its equivalent minimization problem, are consequences of the inequality of Korn's type on a general surface (Thm. 2.6-4), of the uniform positive definiteness of the two-dimensional elastic tensor of the shell (Thm. 3.3-2), of the existence of a0 such that a(y) >_ a0 > 0 for all y e ~ (Thm. 3.3-1), and of the Lax-Milgram lemma, m In Sect. 2.6, we also described how Blouza & L e Dret [1994a, 1994b, 1999] showed that the introduction of new expressions, denoted "~af3(O) and fbaf~(O) (see in]ra), for the functions 7af3(rl) and Pa~(~) affords to consider more general situations, where the mapping 8 need only be in the space W 2, ~176 1~3). For a linearly elastic shell, simply supported along its entire boundary (boundary conditions of clamping along a portion of its boundary can be handled as well, provided they are first re-interpreted in an ad hoc manner), the associated Koiter~s e q u a t i o n s for shells whose m i d d l e surface has little r e g u l a r i t y accordingly take the following form: The unknown ~g, which is now the displacement field of the middle surface, satisfies the variational problem 75~7(w) 9

= L l~e" ~ ~ d y

for all ~ E ~r~c(W),

340

Koiter's equations and other linear shell theories

[Ch. 7

where 1 :=

. a,, + 0 , , 0 . a , ) ,

the given function/5 e E L2(w) account for the applied forces, and a a ~ r , e a r e the usual contravariant components of the two-dimensional elasticity tensor of the shell. Recall that "~a#(0)- 7a#(r/) and tba#(0 ) : pa#(r/) if 0 - ~7iai is such that r / = (~/i) e H i ( w ) • Hi(w) • H2(w). A proof similar to that of Thm. 7.1-1, now based on the inequality of Korn's type on a general sur]ace with little regularity (Thm. 2.6-6), then produces the following existence and uniqueness result: T h e o r e m 7.1-2. Let there be given a domain w in I~2 and an injective mapping 8 E W2'~176 I~a) such that the two vectors aa - OaO are linearly independent at all points of-~. Then the variational problem 79~c(w) has one and only one solution, which is also the unique solution to the minimization problem: ~~ Find ~g such that

~K E ~rK(w ) and jeK( ~ K ) -

inf

~c(~/), where

~e . ~Tv ~ dy.

II

We emphasize that, in this approach, the unknown ~K and the fields ~ are displacement fields of the middle surface, no longer recovered as ~K = ~c,i a~ or ~ -- ~ia z by means of their covariant components ~f,i or r/i. We next derive the boundary value problem that is (at least formally) equivalent to Koiter's variational problem 7~c(w). We only consider here the case where 70 = 7; see Ex. 7.2 for the case where length 3'0 < length 7. ~,~

o

,

Sect. 7.1]

341

The two-dimensional Koiter equations

We also state a regularity result that provides instances where the weak solution (the solution of the variational problem) becomes a classical solution (a solution of the boundary value problem). Theorem

7.1-3. A s s u m e that 7 0 - 7, so that •



(a) If the solution ~ g o] the corresponding variational problem 7~c(w) (Thm. 7.1-1) is smooth enough, it also satisfies the boundary value problem: mafl, ela fl _ b~ba~ma~,e _ ba~nafl, e = pa, e in w, _(na/3, e + b~mr

_ ba(mCf3, elf3) _ pa, e in w,

r

~ - o o~ ~ - O~G,~

~,

where na/3, e := eaaf3~r'eTar(~eK) ,

~3 a aflcrr' epar(r real3, e := --if-

and, for an arbitrary tensor with twice differentiable covariant components n af3, n~l~

:= O ~ n ~ + r ~ n ~

+

na[31a[3 .-- Oa(na[3[[3) + r~(nafll/3 ). (b) A s s u m e that, for some integer m > 0 and some real number q > 1, 7 is of class Cm+4, 0 C cm+4(~; ~3), pa, e E w m + l ' q ( w ) , and pa,~ E w m ' q ( w ) . Then

Ce_K - - ( ~ )

e wm+3'q(~g) x w m + 3 ' q ( ~ ) X wm+4'q(&l).

Proof. For notational convenience, we omit the exponents "e" and the indices " K " throughout the proof, i.e., we let

(: "-- ~k, naft := aaflcrr')'ar(r

maf~ "-- laaflCrrpcrr(~), pi := pi, e 3

342

Koiter's equations and other linear shell theories

[Ch. 7

Assume that the solution ~ is "smooth enough" in the sense that n a/~ e Hi(w) and m a/~ e H2(w). We already saw in the proof of Thm. 4.5-1 that

f ~'='~=.(r

~ - - f~ 4~{(='1,)~. + b.,=',3} d~

for aU ~7 -- (r/i) e H](w) • H](w) • L2(w), hence a ~ortiori for all , E H~(w) • H~o(W)• H2(w). It thus remains to transform the other integral appearing in the left-hand side of the variational equations, viz.,

= ~ ~ real30a/3~3 dy + ~ v/-ama/3(2b~O/3y~ - r~,0~3)dy

+ f~ v~m~(-2b;r~,~ + b~l~ - b ~ ~ ) d ~ , where 17 -- (Yi) e H~(w) x Hlo(w) x H2o(W). Using the symmetry the relation (already established in the proof of Thm. 4.5-1): m a~ = m t3a,

0,v~- ~ r ~ , and the Green formula in Sobolev spaces (see, e.g., Vol. I, Thm. 6.1-9), we obtain

~ ma~pa/3(n)V~ dy - - ~ ~/a(O/3ma~ + r$~mo' + r~,m~')0~ dy

+ ~ v/ama~(-2b~F~,y~ + b~]ay~ - b~bz/3y3)dy.

Sect. 7.1]

343

The two-dimensional Koiter equations

The same Green formula shows that

- f~ ~ ( o ~ , ~ '

+ r~,~ " + r~,,~)o~

dy

= ~ V~( maf~ laf~)Ya dy,

~

~ ~ ~ o ~ , ~'~e ~

-

r'r ~"~'"a~}y'~ dy" -~ ~ ~ { o ~ ( ~ ~) +~,~,,o

Consequently~

Using in this relation the easily verified formula

and the symmetry b~]~ - b~al~ (Thm. 2.5-1), we finally obtain

- ~ ~ { b~b~ m~ - m~ Io~},~ ~y. Hence the variational equations

{~o~~(r

+ ~a ~ p~,(r

p'~i}v~dy - 0

for all y = (vii) E Vg(w) imply that

f

~{(~,

+ b~,~')l, + b~(,~'l,) +p~

+ f~ ~ { b o , ~ o , + b~b~,,~~ - m~

dy

+ p~},~ ~y = 0

for all (y~) C VK(w). The announced partial differential equations are thus satisfied in w.

Koiter's equations and other linear shell theories

344

[Ch. 7

The regularity result of part (b), which is due to Alexandrescu [1994], is left as a problem (Ex. 7.3). m Each one of the three formulations found in Thms. 7.1-1 and 7.13 constitutes the t w o - d i m e n s i o n a l K o i t e r e q u a t i o n s for a line a r l y elastic shell. We recall that the functions ~/a~(~?) and paf3(vl) are the covariant components of the l i n e a r i z e d c h a n g e of m e t r i c and c h a n g e of c u r v a t u r e t e n s o r s associated with a displacement field ~?iai of the middle surface S, the functions a a/3ar,~ are the contravariant components of the t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of t h e shell. The functions n af~,e and m af3,e are the contravariant components of the s t r e s s r e s u l t a n t and s t r e s s couple, or b e n d i n g m o m e n t , t e n s o r fields. As shown in Sect. 6.3, the t w o - d i m e n s i o n a l b o u n d a r y cond i t i o n s of c l a m p i n g ~:,i - 0 ~ : , 3 - 0 on 70 express that the points of, and the tangent spaces to, the deformed and undeformed middle surfaces coincide along the set 8(')'0); cf. Fig. 7.1-1. The functional j~: 9 Vg(w) -+ IR in Thm. 7.1-1 is the twod i m e n s i o n a l K o i t e r e n e r g y of a l i n e a r l y elastic shell. The associated K o i t e r s t r a i n e n e r g y :

n e

-+

~3 aaf3ar' + -~ eO,Tr( ~l) Oa, ( rl ) } v/-a dy

is thus the sum of the strain energy of a linearly elastic el@tic membrane shell (Sect. 4.5) and of the strain energy of a linearly elastic flezural shell (Sect. 6.3)l Showing that this uncanny and eerie "addition" is in fact of the utmost pertinence is the object of the next section. Remarks. (1) In the original derivation of Koiter's equations, the functions n af3'~ and m af3,e found in Thm. 7.1-3 are first defined by means of an ad hoc "two-dimensional variational principle" (Koiter [1970, Sect. 4]); they are then shown to be related to the components craf~'e of the linearized stress tensor field (Thm. 1.6-1) inside the shell by the equations (Koiter [1970, eqs. (4.4) and (4.5)]): n"~, ~ =

F

{a"~, ~ E

Justification of Koitev's equations

Sect. 7.2] m "z''=

S

+

1

345 a i.

e

These formulas justify the terminology "stress resultants" and "stress couples" attached to the functions n af3, ~ and m all' e. (2) Analogous relations can be rigorously derived from the twodimensional equations of a linearly elastic elliptic membrane shell, the functions n aft' e := eaafl~r,e.y~r (~e) being then related to the limit stresses aafl'~(O) by the formulas (Ex. 4.4)

naf3, E _

craf3, e (0) dz~"

(3) In the two-dimensional linear Kirchhoff-Love theory of plates, the "stress couples" are usually defined by the formulas (Vol. I, Thm. 1.7-3) m af3'e -

F z~a af3'e (0) dx~.

Note the change of sign! (4) The functions m aft, e laf3 are instances of second-order covariant

derivatives of a second-order tensor field. (5) Koiter's equations can also accommodate loads and couples applied along the remaining portion 0(7 - 7 0 ) of the boundary of S; see Koiter [1970, eqs. (3.8), (3.9), and (3.13) to (3.15)]. II

7.2.

JUSTIFICATION OF KOITER~S EQUATIONS FOR ALL TYPES OF LINEARLY ELASTIC SHELLS

Consider the same linearly elastic shell problem as in Sect. 7.1. Then the corresponding three-dimensional variational problem 79(f~e) consists in finding u e - (u~) such that (all notations used infra are

Koiter's equations and other linear shell theories

346

[Ch. 7

defined as in, e.g., Sect. 3.1): u e e V(f~ e) -- {v e -- (v~) e Hl(f~e); v e - 0 on r~),

f

AiJkl, eekllt(ue)eill e e j (v e )~/~ dx e e

----fn fi'ev~xfg-gdxe+fr 9

sur ~_

hie' viedre

for all v ~ e V(O~),

where

AiJht, e := )~egij, egkt, e + tze(gih, egfl, e + git, egjk, e), 1

e

,

e

e~llJ(V" ) " = -~(O~v i -]- 0 i v j ) - ri~

e(ve

).

The unknown functions u~ in problem 7~(f~e) represent the covarig g ant components of the displacement field uigZ' of the points of the reference configuration | the functions A ijm,~ denote the contravariant components of the three-dimensional elasticity tensor, the e ( r e ) denote the covariant components of the linearized functions ei]lj strain tensor, and d r ~ denote the area element along the boundary of the set f~e. Consider now a family of such shells, with each having the same middle surface S - 8(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 8(V0) as its middle curve. All the linearly elastic shells in such a family are thus either elliptic membrane, or generalized membrane, or flexural, according to the definitions given in Chaps. 4, 5, and 6. We now show that, in each case, the asymptotic behaviors as ~ --+ 0 of the

average ~ f~-e ue dxl of the solution to the three-dimensional variational problem P(f~') and of the solution r to the two-dimensional Koiter equations formulated as the variational problem 79~c(w) (Thin. 7.1-1) are identical For elliptic membrane and flexural shells, we show in addition that the same property holds, separately for the tangential components ~ f~ u'ao-a'" dx~ and r a and for the normal come aa 3 of the associated displacement ponents 1 fe__eulg3, e dx i and CK, fields.

Justification of Koiter's equations

Sect. 7.2]

347

To this end, we use in an essential way the convergence theorems established in Chaps. 4, 5, and 6, together with slight improvements over former results of Destuynder [1985], Sanchez-Palencia [1989a, 19895, 1992], and Caillerie & Sanchez-Palencia [1995a] (see also Caillerie [1996]) about the asymptotic behavior of the solution of Koiter's equation as e approaches zero. The forthcoming analyses have been recently extended by Xiao Liming [1998, 1999a, 1999b], who likewise justified the time-dependent Koiter equations for elliptic membrane and flezural shells. To begin with, we consider elliptic membrane shells. We follow here Ciarlet & Lods [1996c, Thm. 2.1]. T h e o r e m 7.2-1. Assume that B C g3(~; I~3). Consider a family of linearly elastic elliptic membrane shells, according to the definition given in Sect. 4.1, with thickness 2~ approaching zero and with each having the same elliptic middle surface S = B(-~), and let the assumptions on the data be as in Sect. 4.1; in particular then, 3'0 = 3'. For each ~ > 0 let (u~) e H I ( ~ e) and ~

--(~i~,K) e H~(w) • H~(w) • H2(w)

respectively denote the solutions to the three-dimensional and twodimensional variational problems 7~(~ e) and 79~(w). Let also

denote the solution to the two-dimensional scaled variational problem T~M(W) (Thm. 4.5-1), solution which is thus independent of e. Then

Ii

u ae~ n a'e dz~3 ----+ ~aa a in Hi(w) as e --+ 0, ~ , a aa ~

Caaa in Hi(w) as e --+ 0,

and

1F ~ , g a 3 --+ ffza 3 in L2(w) as e ~ O.

348

[Ch. 7

Koiter's equations and other linear shell theories

Proof. Under the assumptions that there exist constants A > 0 and p > 0 and functions fi E L2(f~) and h i E L2(r+ u r_) independent of e such that Ae = A

and

p~ = p,

f i , ~ ( x ~ ) - fi(x)

for all

x ~ -7r~x E W,

h~,~(~ ~) - ~hi(~)

fo, an

~ - ~

e r ~ u r ~_

(these are the assumptions on the data for a family of linearly elastic elliptic membrane shells; cf. Sect. 4.1) and that 0 E C3(~; I~3), the convergences

if

2-~

ueaga'~ dxea ~

~aaa in Hi(w)

u~g 3 dx~ ~

~3a 3 in L2(w)

and

1 2e

e

as e --+ 0 have been established in Thm. 4.6-1, as corollaries to the fundamental convergence result of Thm. 4.4-1. Th. r r ~ r in H~(~) • H~(~) • L2(~) wa~ ~ t established by Destuynder [1985, Thm. 7.1]; it was also noted by Sanchez-Palencia [1989a, Thm. 4.1] (see also Caillerie & SanchezPalencia [1995a]), who observed that it is a consequence of general results in perturbation theory, as found for instance in Sanchez-Palencia [1980]). We give here a simple and "self-contained" proof. Let a a ~ r .--'-- 2Ap aa~aCrr + 2#(aa,ra~r + aara~Cr) '

~+2#

BF(r

1~ a a ~ r P,rr(r

n):= ~

L(rl) :=

L

fi dx3 + h+ + h i_,

P*~Tiv/~dy, where pi ._ 9

v ~ ( ~ ) := H~(~) • H~(~) • L~(~),

ll,oll 1,w -~" 1,7312,,,,} ~/2

:: Cr

i

1

Sect. 7.2]

Justification of Koiter's equations

349

Recall that there exists a constant ce > 0 such that (Thm. 3.3-2)

It~] ~ < ~ ~ ( y ) ~ ~ a,f3

for all y E ~ and all symmetric matrices (tar3) and that, according to the inequality of Korn's type on an elliptic surface (Thin. 2.7-3), there exists a constant CM such that

i1.11v=. .

a,fl

for all v / = (r/i) E VM(W). Finally, note that the space Vg(w), which here is simply H~(w) x H~(w) x H2(w), is contained in the space

v~(~). By virtue of the assumptions on the applied forces, the solution ~ : of the two-dimensional Koiter equations also satisfies the scaled Koiter equations for an elliptic membrane shell, viz.,

BM(~K, ~) + s 2 B F ( ~ : , v/) = L(~7) for all ~/e Vg(w). Hence letting v / - ~ : in these scaled equations yields the inequality 1

2

1

v~(~)

~

2 0,~ -

a,fl

where

ll il - { 9

Ip'lo, o}'" 2

i

9

This inequality shows that the family ( ~ ) e > 0 is bounded in VM(W) and the families (sPaf3(~:))e>o are bounded in L2(w). Consequently, there exists a subsequence, still denoted (~:)e>o for convenience, and there exist a field ~* G VM(W) and functions p J E L2(w) such that (as usual --+ and ~ respectively denote strong and weak convergences): ~ : --~ ~* in VM(w) and spaf~(~:) --~ p ~ in L2(w). Fix ~/ E Vg(w) in the scaled Koiter equations and let s ~ 0; then the above weak convergences yield BM(~*, ~l) = L(~l). Since the space Vg(w) is dense in VM(w), we conclude that BM(~*, ~l) -- L(~l) for all ~7 E VM(oJ). Hence

r162

Koiter's equations and other linear shell theories

350

[Ch. 7

where r E VM(W)is the unique solution to the scaled problem (Thm. 4.5-1), and the weak convergence

~)M(W)

then holds for the whole family (~r By the inequality of Korn's type on an elliptic surface and by the positive definiteness of the scaled two-dimensional elasticity tensor of the shell, establishing the strong convergence ~ : -+ ~ in VM(W) is equivalent to establishing the convergence

BM(r

- r r

- r -~ O.

Letting r / - ~ : in the scaled Koiter equations shows that

BM(r

r

_< L(r

Hence

o _< B~(r = B~(r

_< L(r

r ~:Ic r

-

-

r -

-

2B~(r

2B~(r

r + B~(r

r + L(r

r

since BM(~, r - - L(~). Noting that the weak convergence ~ in VM(W) implies that

BM(r

-~

r -+ BM((~, ~) and L(r162 -+ L(r

we have thus shown that BM(~eK- ~, ~eg - ~ ) ~ O, hence that ~

-~ ~ in

VM(W).

This convergence clearly implies that ~ , ~a ~ -~ ~aa ~ in H l(w) and ~ , 3a 3 -~ C3a 3 in L 2 (w). 1

The convergence results of Thm. 7.2-1 have been improved by Mardare [1998b, Thm. 5.1], who showed that I!r

-

r

=

0(81/5),

Justification of Koiter's equations

Sect. 7.2]

351

and by Lods & Mardare [1998b, 1999c], who showed that

1F

u e dx~

-

r215215

-

O(g:l/5)

9

Remark. Under the assumptions of Thm. 7.2-1, the function ~'~,K thus "looses its boundary condition" as ~ approaches zero. This phenomenon, together with its accompanying boundary layer, can be already observed on a simple one-dimensional model of Koiter's equations (Ex. 7.4). As already noted (Sect. 4.6), a similar "loss 1 of boundary condition" is shared by the average 2ee

e u~ dx~ as s

approaches zero.

I

We next turn our attention to generalized membrane shells of the first kind. We follow here Ciarlet & Lods [1996d, Thins. 6.1 and 6.2]. In the same way that we required the applied forces to be "admissible" (Sect. 5.5) in order to carry out our asymptotic analysis of the solutions of the corresponding three-dimensional equations (Sect. 5.6), we need to assume that the applied forces enter Koiter's equations in such a way that the corresponding scaled linear forms are continuous with respect to the norm l" IM of the "limit" space V~M(W) and uniformly so with respect to ~. More specifically, we set the following definition (notice the analogy with that given in Sect. 5.5): Applied forces are a d m i s s i b l e for t h e t w o - d i m e n s i o n a l K o i t e r e q u a t i o n s if there exist functions r _ ~ a E L2(w) such that, for each s > 0, the right-hand side in Koiter's equations cart also be written as

p i' e~Ti~ d dy - 6 f~

n-

e

Remark. For simplicity, we assume here that the scaled linear forms (denoted LM in the next proof) are independent of s. But the conclusions of the next theorem would be unaltered under the more general assumption that, for each s > 0,

pi'e~Ti%~dy - e fw qoa~(s)Va~(17)v~dy for all r / = (r//) e VK(w),

352

Koiter's equations and other linear shell theories

with functions ~ ( e ) ~ L2(w) converging strongly to ~ as e approaches zero.

[Ch. 7

in L2(w) 1

T h e o r e m '/.2-2. Assume that 0 E C3(~; ]R3). Consider a family o/linearly elastic generalized membrane shells of the first kind, according to the definitions given in Sect. 5.1 and 5.4, with thickness 2e approaching zero, with each having the same middle surface S = 0(-~), with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(7o) as its middle curve, and subjected to applied forces that are admissible for both the three-dimensional equations (Sect. 5.5) and the two-dimensional Koiter equations, the/'unctions ~oa# C L2(w) coinciding in addition with those found in Thm. 5.6-1. For each e > O, let

u e e Hl(f~ 6) and r

e Hi(w) x Hi(w) • H2(w)

respectively denote the solutions to the three-dimensional and twodimensional variational problems 7~(f~~) and 7~c(w). Let also

r ~ V~M(W) "-- completion of V(w) with respect to [. IM, where v(~)

:= { . = (w) e a l ( ~ ) ; .

= o on ~0},

a,/3

denote the solution to the two-dimensional scaled variational problem 7:'~M(W) (Thin. 5.7-1), solution which is thus independent of e. Then

u ' dx~ ~

r in VUM(W) as e ~ O,

r

r in V~M(a,) as e --+ O.

~

Proof. Under the assumptions that 0 E C3(~; I~3) and that the applied forces are admissible in the sense of Sect. 5.5, the convergence

1S e u ~ dx~ ~

2~

r in V~M(W)

Justification of Koiter's equations

Sect. 7.2]

353

as e -+ 0 has been established in Thm. 5.8-1, as a corollary to the fundamental convergence result of Thm. 5.6-1. The rest of the proof is an elaboration over Caillerie & SanchezPalencia [1995a, Thm. 4.5], who established the weak convergence ~ : --~ ~ in V~M(W) as e --+ 0. In particular, we establish here that this convergence is strong. Since the space Vg(w) is dense in the space V(w) with respect to the norm t1" l]z,~ and there exists c such that IrllM~ _< cllrlliz,~ for all rl e V(w), the space VK(W) is dense in V(w) with respect to I.I M and thus the space V~M(W) is also the completion of Vg(w) with respect

to I Let B~M and L~M denote the unique continuous extensions from V(w) to V~M(W) of the bilinear and linear forms BM and LM defined by

LM(17) "= L ~~ The applied forces being admissible for the two-dimensional Koiter equations, their solution ~ : satisfies the scaled Koiter equations for a generalized membrane shell, viz., BM(r

~ ) + s2Bv(r

Y) - LM(y) for all y E VK(w),

where

1 L aa~r Hence letting rI - ~ : in these scaled equations yields the inequality (the constant ce stems from the positive definiteness of the scaled two-dimensional elasticity tensor of the shell; cf. Thm. 3.3-2):

+ where

1 a,/3

2 }z/2 9 fILM11 :-- {Ea,~IWa~Io,~

ilLMIIICki M, This shows that the family

(~:)~>0 is bounded in the space V~M(W) and the families (spaf3(~eg))e>O are bounded in L2(w).

354

[Ch. 7

Koiter's equations and other linear shell theories

Consequently, there exists a subsequence, still denoted (r for convenience, and there exist r e V~M(W) and p ~ e L2(w) such that (as usual ~ denotes weak convergence): r

---' r in V~M(W) and ep,~(r

~ p-~ in L2(w).

Fix y E VK(W) in the scaled Koiter equations and let e --+ 0; then the above weak convergences yield B~M(r *, ~) -- LM(y). Since VK(W) is dense in V~M(W), we conclude that B~M(r *, y) -- L~M(y) for all y E V~M(W). Hence

r162

where ~ e V~M(W)is the unique solution to the scaled problem 7~M(W) (Thin. 5.7-1), and the weak convergence r

=

r in V~M(W)

then holds for the whole family (r162 By the positive definiteness of the scaled two-dimensional elasticity tensor of the shell and by the definitions of the norm I" ]M and of the bilinear form BM and of its extension B~M, establishing the strong convergence ~ --~ ~ in V~M(W) is equivalent to establishing the convergence

B~(r Letting rI

=

- r r

- r ~ o.

in the scaled Koiter equations shows that

~c

Bu(r

r

_ Lu(r

Hence

o 0, and let 0 E e3(~; R 3) be an injective mapping such that the two vectors aa = OaO are linearly independent at all points of -~.

Then problem 79~r

has one and only one solution.

II

The variational problem 7~v(w) is, at least formally, equivalent to a boundary value problem, which is again a "uniformly" and "strongly elliptic" system in the sense of Agmon, Douglis & Nirenberg [1964]. Accordingly, the regularity of its solution can be established as the regularity of the solution of Koiter's equations (Ex. 7.3); see Iosifescu [1999]. In the same manner that Blouza & Le Dret [1994a, 1994b, 1999] have generalized Thm. 7.1-1 to "Koiter's equations for shells whose middle surface has little regularity" (Thm. 7.1-2), Slouza [1997] has extended Thm. 7.4-1 to Naghdi's equations ]or shells whose middle surface has little regularity (the mapping 0 need only be in the space

R3)).

Nonhomogeneous and anisotropic linearly elastic materials are likewise amenable to Naghdi's approach. The existence and uniqueness of the corresponding two-dimensional Naghdi's equations can be treated as in Thin. 7.3-1; see Figueiredo & Leal [1998]. The corresponding infinitesimal rigid displacement lemma is due to Coutris [1978].

Naghdi's equations are as much favored as Koiter's for analyzing the locking phenomenon and membrane locking, briefly described

Sect. 7.5]

Other linear shell theories

367

in Sect. 7.3; see Hughes & Franca [1988], Bathe, Brezzi & Fortin [1989], Pitk~iranta [1992], Lyly, Stenberg & Vihinen [1993], Arnold & Brezzi [1997a, 1997b], Bramble & Sun [1997], Suri [1997], Gerdes, Matache & Schwab [1998], Chapelle & Bathe [1998a], Chapelle & Stenberg [1998]. 7.5.

OTI-IER LINEAR

SHELL THEORIES

Linear "shallow" shell theories are treated separately (Sect. 7.6). B u d i a n s k y - S a n d e r s theory. Sanders [1959] and Koiter [1960] have proposed a linear shell theory akin to Koiter's, where the covariant components Pat3(r/) of the linearized change of curvature tensor BS (r/) of the B u d i a n s k y are replaced by the covariant components Pat3 S a n d e r s linearized change of c u r v a t u r e tensor, defined by BS

1

The remaining terms in the equations are otherwise identical to those in Koiter's equations (Sect. 7.1). BS(r/) , rather than The interest of using the modified functions Pa[3 the "genuine" functions pail(r/), has been discussed at length in Budiansky & Sanders [1967] and, for this reason, the resulting theory has become known as the Budiansky-Sanders theory (see also the commentary in Koiter [1970, Sect. 7.5]). More recently, Destuynder [1985] has clearly shown how this theory can be derived from three-dimensional linearized elasticity, again on the basis of two a priori assumptions, both of a geometrical nature (one of them being the linearized Kirchoff-Love assumption; cf. Sect. 7.1), thus providing a mathematical justification of this theory. Remarks. (1) A nonlinear Budiansky-Sanders theory, proposed by Destuynder [1982, 1985], is briefly presented in Sect. 11.2. Bs (r/) and the equivalence (2) The definition of the functions Pail between the equations

(,1)

Bs

= Pa~ (r/) - 0 in

and "fail(r/) = Pat3(r/) = 0 in w"

together imply that the ezistence and uniqueness theory for Koiter's equations (Sects. 2.6 and 7.1) extends almost verbatim to the Budiansky-Sanders equations. II

368

Koiter's equations and other linear shell

theories

[Ch. 7

H i e r a r c h i c s h e l l t h e o r i e s . The underlying principle in a hierarchic shell theory consists in minimizing the three-dimensional energy of a linearly elastic shell, expressed in terms of its "natural" curvilinear coordinates (yl, y2, x~), over a subspace of displacement fields of a special form: Each one of their covariant components is a finite sum of products of functions of (Yl, y2) (to be determined through the minimization process) times linearly independent functions of x~ (typically, ad hoc orthogonal polynomials). Increasing the number of linearly independent functions of the transverse variable produces a "hierarchy" of presumably increasingly accurate approximations. Due credit should be given in this respect to Vekua [1986, Chap. 1], for one of the earliest attempts to put such an approach for shells on a sound mathematical basis. Hierarchic theories are especially advocated as efficient numerical methods: In particular, they have proved to be quite successful for the numerical approximation of plate problems; see Szabo & Sahrmann [1988], Babu~ka & Li [1991], Babu~ka, Szabo & Actis [1992], Sabu~ka, d'Harcourt & Schwab [1993], Schwab [1994, 1996], Schwab & Wright [1995], Babu~ka & Schwab [1996]. They will certainly be increasingly used for the numerical approximation of shell problems~ notably for their abilities to handle multi-layered shells, also called composite or laminated shells, boundary layers, or the membrane locking phenomenon (Sect. 7.3); see notably Oden & Cho [1996], Actis, Szabo & Schwab [1999]. L i n e a r shell t h e o r i e s b a s e d o n t h e m e t h o d o f i n t e r n a l c o n s t r a i n t s . The linearized Kirchhoff-Love assumption (Sect. 7.1; see

also Ex. 7.1(2)) can be considered as an internal constraint imposed ab initio on the displacements that a shell can undergo. In this approach, first advocated by Podio-Guidugli [1989] for linearly elastic plates, then by Podio-Guidugli [1990] for linearly elastic shells~ special care must be exercised for the determination of the resulting two-dimensional constitutive equation, through a careful distinction between "reactive" and "active" stresses. " I n t r i n s i c ~ l i n e a r s h e l l t h e o r y . An "intrinsic" approach to linear shell theory has been proposed by Delfour & Zoldsio [19951 for modeling shells whose middle surface is the entire boundary r of a domain ~ C I~3. This approach makes an essential use of the "tangential differential calculus" developed in the book of Sokolowski

Linear shallow shell theories

Sect. 7.6]

369

& Zol6sio [1992] and of the "oriented distance function" A" ~3 -4 I~, defined by A ( x ) - d(x, r ) i f x e {I~a - f~} and A(x) = - d ( x , F) if x E 12, also used in Delfour & Zol6sio [1994, 1998] in a different context. After integrating the three-dimensional energy across the thickness and making ad hoc simplifying assumptions, M.C. Delfour and J.P. Zol6sio derive linear shell theories that bear strong resemblance with those of W.T. Koiter and P.M. Naghdi. An interesting feature of this approach is that local bases are not used. This approach has since then undergone manifold extensions, which often parallel the asymptotic analyses of the previous chapters. See notably Delfour & Zol6sio [1997a, 1997b], Delfour [1998,

1999]. 7.6.

LINEAR

SHALLOW

SHELL THEORIES

Linear shallow shell theories in Cartesian coordinates are treated at length in Vol. II, Chap. 3. Accordingly~ the additional commentary and bibliographical notes found in this section apply mostly to linear shallow shell theories expressed in curvilinear coordinates. According to the definition proposed by Ciarlet & Paumier [1986] in the nonlinear case, then justified by a convergence theorem as the thickness approaches zero by Ciarlet & Miara [1992a] in the linear case, a shell is s h a l l o w if the deviation of its middle surface S ~ from a plane is of the order of the thickness, i.e., if

S ~ -- Os (~), where

and 0 : ~ -4 R is a smooth enough function that is independent of e. A w o r d of c a u t i o n . This specific "variation of the middle surface with e" thus constitutes an additional assumption on the data, special to linear and nonlinear shallow shell theory, m

Koiter's equations and other linear shell theories

370

[Ch. 7

As shown by Busse, Ciarlet & Miara [1997], who use the same definition of "shallowness", the two-dimensional equations of a linearly elastic clamped shallow shell "in curvilinear coordinates" can be given a rigorous justification by means of a convergence theorem as the thickness goes to zero. As the proof essentially resembles that given in Cartesian coordinates by Ciarlet & Miara [1992a] (see also Vol. II, Sect. 3.5), it is not reproduced in this volume. We simply list the limit equations that are found in this fashion, when they are expressed as a minimization problem: Let baf3~r,e .-'- 4~e# e ~ a ~ r $e + 2#e p,,e :=

f

:=

sh,

+ 2tze(~a~Or + ~ar~f3~),

fi, e dx~ + h~_~ + h i, ~

"

e

4I

+

--

-

1

and let a i' e designate the vectors of the contravariant bases along the middle surface S e. Then the unknown is the vector field ~e = ( ~ ) , where the functions ~ : ~ --+ R are the covariant components of the displacement field ~ a i'e of S e, and (~e minimizes the energy jsh, e defined by

jsh ' e(rl) . - 2

/ eba~er, e_.h,e ecrr

. .h,e ( y ) - ] - -~- ba/3~r,e 0qry30afj~73 (y)ea/51

dy

-{fwPi'e?~idy-fwqa'e~adYl, over the space (the same as for Koiter's equations; cf. Sect. 7.1): V K ( 0 g ) :-- {O -- (~7i) 6 H l ( w ) x H l ( w ) x H 2 ( w ) ;

~7i -- 0v~3 -- 0 Oil 70}"

An inspection of this minimization problem reveals that, even though it is expressed in curvilinear coordinates, it "resembles more that of plate (Vol. II, Chap. 1) than that of shell"! For the contravariailt components of the metric tensor usually found in the twodimensional elasticity tensor are now replaced by Kronecker deltas, the area element along the middle surface is replaced by dy, and finally, the components of the linearized change of metric and change

Sect. 7.6]

371

Linear shallow shell theories $h~ s

of curvature tensors are replaced by the functions ear 3 (v/) and 0afar/3 where neither the Christoffel symbols nor any components of the curvature tensor of S e are to be found. The equations found in this fashion constitute Novozhilov's model of a shallow shell, so named after Novozhilov [1959]. These equations, which were first analyzed by Shoiket [1974], were given a first justification by Destuynder [1980] for special geometries. As shown by Andreoiu [1999a], it is a reassuring circumstance that the limit displacement fields found in either Cartesian or curvilinear coordinates, though not identical vector fields, are nevertheless "essentially the same", i.e., their components agree "to within their first orders", once they are expressed in a same basis. The asymptotic analysis of the corresponding eigenvalue problem has been carried out in Cartesian coordinates by Kesavan & Sabu [1999b]; there is no doubt that it could be similarly carried out in curvilinear coordinates. The exponential nature of the boundary layers that arise in linearly elastic shallow shells is analyzed in Pitk/iranta, Matache & Schwab [1999]. Models of multi-layered, or composite~ linearly elastic shallow shells, found in particular in hulls of sailboats, have been obtained by Kail [1994] by means of the method of formal asymptotic expansions. The control of vibrations in linearly elastic shallow shells by means of piezo-ceramic actuators is studied in detail in Banks, Smith & Wang [1995, 1996]. Other definitions of "shallowness" have been proposed, which often make explicit reference to the curvature of the middle surface. For instance, Destuynder [1985, Sect. 1] considers that a shell is "shallow" if 7/= ep for some p >_ 2, where the other "small" parameter is the ratio of the thickness 2e to the smallest absolute value of the radii of curvature along the middle surface, p = 2 corresponding to Novozhilov's model. In this direction, see also Vekua [1965], Green & Zerna [1968, p. 400], Gordeziani [1974], Dikmen [1982, p. 158].

372

[Ch. 7

Koiter's equations and other linear shell theories

EXERCISES

7.1. All the notations used in this problem should be self-explanatory. The Kirchhoff-Love assumption for a shell states that all points lying initially on a given normal to the middle surface remain on a single normal to the deformed middle surface and that the distance from any point of the shell to the middle surface remains unchanged. Consider a shell with a reference configuration O ( ~ e) equipped with its "natural" cuxvilinear coordinates (yl, y2, x~) C ~e and let g~,e denote the vectors of the corresponding contravariant bases in O(~e), where fF = w• - e, e[. Thus a displacement field vige i,~ of the set O ( ~ e) satisfies the Kirchhoff-Love assumption if and only if

where ~Tia~9 denotes the restriction to x~ = 0 of the field Ve-.i i Y' e and a3(r/) is the "usual" vector normal to the deformed middle surface

(0 + (1) Show that a displacement field v~g i,e of (9(fi e) satisfies the Kirehhoff-Love assumption if and only if the covariant components gi~(v e) of the metric tensor of the associated deformed configuration, assumed to be equipped with the same eurvilinear coordinates as those of | are of the form

g~/3(v e) -- aa/3(rl) - 2xlba/3(rl) + (xl)2b~(rl)bf3o.(17) and giea(ve)

--

~i3,

where aa~(r/), bad(r/), and b~,(r/) denote the covariant and mixed components of the metric and curvature tensors of the deformed middle surface (0 + ~Tiai)(~). (2) k displacement field ui "e..~,, of @( ~ ) satisfies the linearized Y Kirchhoff-Love assumption if only the linear terms with respect to r/ are retained in the difference { a z ( r / ) - a3}. Show that such a displacement is of the form (see, e.g., Bernadou & Boisserie [1982, eq. (1.3.19)]): veni, e --

a i -

i(O

v3 + b13a 71 )a a

7.2. Assume that the boundary 7 of w and the functions pi, e are smooth enough and that length 7o < length 7. Show that, if the solution ~ c - ( ~ , i ) to the variational problem 79~(w) (Thin. 7.1-1)

373

Ezercises

is smooth enough, it is also a solution of the following boundary value problem:

mafi}, e laj3 +

_

_

b~bat3ma[3,e _ ba~na[3, e = pa, e in co, -

iie, K

-- Ou~3,e K

-

i.

-- 0 on

70,

ma~'~uau~ --0 on 71, (m~Z'~l~)~,z + O ~ ( m ~ Z ' ~ r Z ) -- 0 on 7~,

(n az'e + 2ba~m~Z'6)vZ - 0 on ")'1, where 71 := 7 - 3'0, (ua) is the unit outer normal vector along 7, T1 := --u2, T2 := Ul, and 0~0 := ra0a0 denotes the tangential derivative of 0 in the direction of the vector (Ta). Remark. It is instructive to compare these equations with those of a linearly elastic plate (Vol. II, Thms. 1.5-1, 1.5-2, and 1.7-2). 7.3. The following problem shows, after Alexandrescu [1994], how to establish the regularity (announced in Thm. 7.1-3 (b)) of the solution of the two-dimensional Koiter equations for a linearly elastic shell. It is assumed throughout this problem that 70 = 3', and in (1), (2), and (3) that the boundary 7 is of class C4 and the mapping 0 is in the space C4(~; R 3). (1) Show that the linear system of partial differential equations found in Thm. 7.1-3, which is of the second order with respect to the unknowns ~ : , a and of the fourth order with respect to the unknown ~c, 3, is "uniformly elliptic" and satisfies the "supplementing condition on L " and the "complementing boundary condition" in the sense of Agmon, Douglis & Nirenberg [1964]. Remark. These properties are shared by the systems of partial differential equations found in Thm. 2.7-2 and in Ex. 4.2. (2) Show that the same system is "strongly elliptic" in the sense of Ne~as [1967, p. 185]. Using Ne~as [1967, Lemma 3.2, p. 260], infer from this property that the solution r - (i~,i) to the variational problem T'~c(w ) (Tam. 7.1-1), which belongs to the space Hlo(W) • H~(w) • H2o(W) since ")'0 = ~' by assumption, satisfies

374

Koiter's equations and other linear shell theories

[Ch. 7

if pa, e E H i ( w ) and pa, e C L2(w). (3) Using Geymonat [1965, Thm. 3.5], shows that

~K

--(~K,i)

e w3'q(o3) X w3'q(og) x w4'q(o3)

ifpa'e E w l ' q ( w ) and p3,e C Lq(w) for some q > 1. (4) Assume that, for some integer m >__ 1 and some real number q > 1, 7 is of class Cm+4, 8 E Cm+4(~; I~3), pa, e E Wm+l'q(w), and pa, e E wm'q(w). Show that

~eK "-(~K,i) e Wm+3'q(~g) x Wm+3'q(og) x wmT4'q(og). Hint: For (4), use Agmon, Douglis & Nirenberg [1964].

7.4. As shown by Sanchez-Hubert & Sanchez-Palencia [1993, p. 55] (see also Leguillon, Sanchez-Hubert & Sanchez-Palencia [1999]), the following simple, yet illuminating, two-point boundary value problem can be viewed as a convenient one-dimensional model of Koiter's equations, as regards in particular the behavior of their solution as approaches zero in the situations covered by Thms. 7.2-1 and 7.2-2. The space H - m ( 0 , 1) denotes the dual space of H~n(0, 1). Given f E H-2(0, 1), let u e E/-/2(0, 1) denote for each e > 0 the solution to the boundary value problem: ~2

d4u ~

d2u e

dx 4

dx 2

= f in ]0, 1[,

ue(0) - (ue)'(0) - ue(1) - (ue)'(1) - 0. (1) Assume that )e E L2(0, 1). Show that u ~ -+ u ~ in H~(0, 1) as e -+ 0, where u ~ E H~(0, 1) is the solution to the boundary value problem d2u o

dx2 = I in ]0, 1[, -0.

(2) Compute explicitly and plot the solutions u ~ corresponding to f = 1. Show that boundary layers appear in the derivative (ue) ~ as approaches zero. Remark. Such boundary layers reflect that the boundary conditions (ue)~(O)= (ue)~(1)= 0 are "lost" at the limit.

Ezercises

3'[5

(3) Let f r where r denotes the derivative of the Dirac distribution at x - ~. 1 Verify first that it e H -2(0 , 1) , but that f ~ H - 1 (0, 1); then show that -

-

u~(x)-+x

for each

0_ 0 be chosen as in Thm. 3.1-1. Then

gij (e)

-

-

a ij + e x 3 g ij' 1 + O(e2),

aiJ .= a i . a j

r,5(~)

-

r ~,o

-o~

I

:__ 2aaCrb~ ~

gi3 , 1 = 0 ,

r,~ 0 + ~,~r,jp, 1 + o(~), where .

.__

gaf3,

,

where

~.o

~..o T~cr, 1

- b ; l o , - o ~ :=

-o~

1" cr

-=-b~b,,

3,0

up,0

r

a3 = ' 3 3

::

0~

r

3,1 rp, 1 a3 = ' 3 3 ::

0,

and finally, g(e) = a + O(e), for all 0 < e _< co, where the functions a #, ba~, b~, r ~af3, b~]a, and a are identified with functions in C~ and the order symbols O(e) and O(e 2) are meant with respect to the norm i[ " [[0,c~,~ defined by i1~110 oo ~

:=

sup{lw(m)l; m e n )

Proof. The asymptotic behavior of each function gZ3(e) immediately follows from the relations ~ a ( g ) _ act ~ gx3b~atr + O ( g 2 ) ,

established in the course of the proof of Thm. 3.3-1. All the other n relations were already proved in the same theorem.

Sect. 8.6]

The method of formal asymptotic ezpansions

413

Observe that the notation a i1 is consistent with that used for the contravariant components a af3 -- a a . a f3 of the metric tensor of the surface S; note also that a i3 = ~i3. Our second result, which is a restatement of Thm. 3.3-2 (b), gathers all the "mechanical" preliminaries needed in the sequel, in that it describes the behavior as ~ --+ 0 of the scaled contravariant components AiJkt(e) of the three-dimensional elasticity tensor (defined in Thm. 8.4-1). Note that their limits for e = 0 are again functions of y E ~ only. T h e o r e m 8.5-2. Let w be a domain in I~2, let 0 C g3(~; i~3) be an injective mapping such that the two vectors aa are linearly independent at all points of-~, and let ~o > 0 be chosen as in Thm. 3.1-1. Then the contravariant components AiJkt(e) - AJikt(e) -- AktiJ(e) of the scaled three-dimensional elasticity tensor satisfy

AiJkt(e)v/g(e ) = AiJkt(0)v/-d + 6B ijkl,1 + eZBiJkt,2 + o(62), where

Aa~'rr(0 ) : - Aaa~a ,rr + #(aa'ra ~r + aara~'r), Aaf333(0) := Aa aft, AaZ'r3(0) "- pa a'r, A3333(0) := )~ + 2/z, A

(0)

-

A

333 (0) " - 0,

for all 0 < ~ - 3 N - 4 the linear form defined by

Lr(v) := fn f i ' r v i ~ d x

+ fr+ur_

hi, r + l v i v f a c ~ ,

and it is always understood that the functions/,,r and h i'r+l belong to the spaces L2(12) and L2(r+ U r _ ) and are independent of e. (iv) Assume that N >_ O. Since the lowest power of s in the left-hand side is e -3N-4, we are naturally led to first try

1

f i ( e ) __ e 3N+4

1h fi,-3N-4 and h~( e ) - ~e3N+ 3 i, -3N-3

Then the cancellation of the coefficient of e -3N-4 leads to the equation (the functions ~..,3113 and F3113 defined in (iii)):

f n ( )~ + 2p ) E 3-1123N- 2F3 t--1~- 2(v ) v/'d d x - L-3N-4(v )

Sect. 8.7]

The leading term is of order zero

419

for all v E W(fl). Since E -2N-2 3113

_

-

lamnOau~nN O3u-~N and F31-~3N-2(v)- amnOaUmN O3vn, 2

we must have

L - 3 N - 4 ( v ) -- / n f i ' - 3 N - 4 v i ~ d x

-t- ~ + u r - h i, -3N-3 Vi V~ dr - 0

for all v E W(f~) that are independent of x3. Consequently, the first requirement (that there be no restriction on the applied forces) implies that we must let fi,-3N-4 = 0 and h i'-3N-3 = O. Letting v - u - N in the resulting variational equations then shows that

/12 E3''3-2N-2F3,,3-N-2 ('tt -N) ~ dx - -~l / (amnO3u~O3unN)2~/a dx - O. Since the symmetric matrix (a ij) is positive definite, we conclude that

03 u - N - (03urn N) - 0 in ~, i.e., that u - N is independent of x3. We thus infer that E3~I2N-2 -- 0 ~nd F ~ l ~ - ~ ( ~ ) - 0 fo~ ~11 ~ e W ( a ) . Cancelling the coefficient of e -3N-4 thus yields the following relations (as usual, any function defined on ~ that is independent of x3 is identified with a function defined on ~)"

'U-N E W ( w ) : = E ~llJ -~-2

{71 = (~i) E wl'4(og); ~ = 0 on "Y0},

: 0 in a ~ d ~ ~ - 2 ( ~ )

_ 0 fo~ ~11 ~ c W ( a )

since ~3113~-2N-2= 0 and __F3113-N-2(v)-- 0 and the leading terms in the highe~ th~n ( - 2 N 2) ~na ( - N 2), ~especti~ly. Since E~-I~;-1 : 0 (the leading term in the formal expansion of E~ll~(~; ~(~)) ~s of o~de~ - 2 N ) ~ d ~1~] ~ - ~ : 0 ( s ~ 0 ~ - ~ - 0, 1 each factor of e2N+ 1 in the expansion of Eall3(e; u(e)) vanishes because it contains some derivative 03u~ N and the leading term in the expansion of E3ll3(e; u(e)) is of order strictly higher than ( - 2 N - 1)), we also have E -2N-1 = 0 in f~.

420

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

[Ch.

8

Our next try is thus

f i ( s ) _ s 3N+3 1 f , -93 N - 3 and hi (e) - saN+ 1 2 h "9- 3 N - 2 . The cancellation of the coefficient of s -3N-3 then yields the equations (the functions AiJm(O) are defined in Thin. 8.5-2)"

fft AiJkl (O)F~h-[]21N-1Fi~lT-2(v)v/-a dx

-

-

L - 3 N - 3 (V )

for all v E W(f~) 9 But since D?-2N-1 -"~klll - - 0, we must let f i , - 3 N - 3 __ 0 and

h i'-3N-2 = 0 (first requirement) and accordingly try ]i(s)

_

1 ~3N+2 f~'9 - 3 N - 2

1 h i, - 3 N - I and hi(e) = e 3 N + 1

in which case the cancellation of the coefficient of s - 3 N - 2 yields the equations

f

-

for all v E W ( ~ ) . But s i n c e F / H T - 2 C v ) -- 0 for all v C W ( ~ ) , we must l e t f i , - 3 N - 2 = 0 and h i,-3N-1 = 0 (first requirement). (v) Assume that N > 1. Our next try being thus

1 ft,-3N-1 9 f i ( e ) __ e 3N+1 and hi (e) - - -1~ h ' '9- 3 N the cancellation of the coefficient of S - 3 N - 1 in the variational equations of problem 7~(e; ~) then yields the equations

fn AiJkl(O)E-2NF-N-l(v)x/~dz kill i115

-

L-3N-I(v )

-

for all v E W(f~), where

1 mn - N ~.2 N

"o11

-2N E3113

-N

F-N-I(v)

~llf3

-- O,

iamnu-N u-N =

.,llo

iamn -- 2

1

mn

-N

-

.11 ,

-N -N ~tmll3UnJl3'

=

-N O am . Umlt3

v.

,

Sect. 8.7]

421

The leading term is of order zero

N being those defined in (iii); recall that 03Un N -- 0 the functions u -mtli by (iv) and that we assume N > 1 (otherwise some functions, such as E~I~;, have different expressions when N = 0; cf. (iii)). Letting v E W(f~) be independent of x3 then shows that we must let f i , - 3 N - 1 = 0 and h i ' - 3 N = 0; hence / n A i j k t l a ~ E - 2 N F - N - l (v )v/-d dx - 0 x"J kllg illJ

Let the field w N _ (w N) be defined for all

for all v C W(f~). (y, x3) C f~ by

Wm N .___ U~nlV-k-1 _

O -N (1 + X 3 ~) lp ,m3 Up

T h e n w N E W(f~) because both u - N and u - N + I are assumed to be in the space W(f~) (this double assumption is thus crucial!). Furthermore, 03w N = Umll3 - N , so that

F-fIN3-1( w N) - Ea-l~ ~

-2N

and F 3 ~ -I (w N) - 2E3113 .

Letting v - w N in the last variational equations thus shows that

faAijkl(o~E

- 2 N F - N - l (wN)v/-d dx - 0, J kilt illJ

where 2)~amnE-2N

Aijkl(a~"-2NF-N-I(wN)=

~''J~kll/

illJ

mlin

- 2 N -b 4 a t o n e - 2 N rz'-2N E3tl3 P roll3 "e'nll3 "

Since amnE_2N

-

1 a ija mnu -Nu -N

rnlln -- 2

> 0 in f~

(by (ii))and

1 mn -N -N _ m n r r t - 2 N rrw-2N -2N E3113 -- -~a Umll3Unll3 >_ 0 and a "~'ml13"C'nll3 >_ 0 in

(the matrix (a ran) is positive definite), we conclude that a m

hence that

n

rry - 2 N

rrv - 2 N

"~ml13 aWnll3

E-2N

-- 0 in f~,

roll3 = 0 i n f l .

422

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

[Ch. 8

1 mn -N -N In particular then, E3~122v- ~a umll3Unll3 = 0 and thus

-N

Umll3 - -

O,

(vi) Assume that N > 2 (the case N - 1 is considered separately; cf. (vii)). Our next try being thus f i ( e ) .._

_ _1 ~ ] , ,. - 3 N and

hi

~s 3 N1h_

(r

1

i, -32v+t

the cancellation of the coefficient of s -aN in the variational equations of problem :P(e; ~) then yields the equations (note that two terms are needed here from the expansions of the functions AiJkt(e)v/g(e); cf. Thin. 8.5-2)

E_2N+IF_N_ 1

~kllZ "~llJ

+ f• BiJkI'IE-2NF-N-lhIIt il1r

kilt

i11i

(v)dx = L-aN(v)

for all v E W(fl), where

1amnu_

~-~

= ~

~,l-i~ ~ -

o by

N _ -N

~llo~.ll, '

(~), 1 mn -N VOSVn,

F~l-i~-~(~) - o by (~), F -N(v) "11~

F___N (.

)

lamn

--

-IV

- N

(U..llaVnll~ + unll~ Vmlla)

a m n u - N + I dO V

the last expression of F~N3 (v) being valid only if N _> 2 (the expressions of Fa]IN(v ) are not needed since Aaaar(0) - 0 and E~I~N -- 0). N 1 Noting that Fa~la(v) -- ~3~3N ( v ) -- 0 if C93V -- 0 we thus conclude that the above variational equations reduce to

fo A~176

r

- L-~(~)

Sect. 8.7]

The leading term is of order zero

423

f o r all v E W(f~) t h a t are i n d e p e n d e n t

of x3. Since each t e r m in is c u b i c with respect to the func-

the s u m A a # ~ r ( O ~ E - 2 N F - N ( v )

N tions u -mlla' the l i n e a r i z a t i o n t r i c k (second requirement) implies t h a t

-- 0 for all v E W(f~) t h a t are i n d e p e n d e n t o f z a . Hence we m u s t let f i , - Z N = 0 and h i ' - a N + l -- O. Since u - N is independent of x3 by (iv), we may let v - u - N in the last variational equations. This gives L-aN(v)

~I-adz = O,

since F - g ( u - N ) _ 2 E - 2 N

But

A a#'rr (0) - )~a af~ a 'rr + # ( a a'r a ~r + a ar a fi~

( T h m . 8.5-2) and thus 2N

1 mn

E~-llfl -- ~ a

-N

-N

UmllaUnllf3 - 0

in f~

(to reach this conclusion, observe that aatrafart~rta~ >_ 0 and t h a t - 0 only if taf~ - 0 by (ii)); these relations in t u r n imply t h a t aa~afart~ta/3

u -N

mll~

-0

By definition (cf. (iii) and T h m . 8.5-1), N - ~pp, a/30up- N -- Oa u/3- g -- r ~a~ U~ N -- ba/aU3

u -~lla N _

Oau~N

-N uall~

0 ~ u ~ N _ r~,p, ~ 3 Oup- N __ OaU3 N .jr b ~ u ; N

Let ~i " - u i N I z s = O 9 T h e n ~i C Wl'4(w) since u~-N E Wl'4(f~) and 0 3 u [ N - 0 in f~ and ~i - 0 on q'0 since u~-N - 0 on r0. The above relations combined with the Gaul] and Weingarten formulas (Thm. 2.3-1) t h e n imply t h a t O a ( ~ i a i) - 0 in w, hence t h a t ~i - 0. We have thus shown t h a t u - N - 0 for all N > 2. o

(vii) F i n a l l y , a s s u m e t h a t N t h a t now

1. The o n l y difference from (vi) is mn

0

03 Vn"

424

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

[Ch. 8

But since the arguments that led in (vi) to the conclusion that u - N - 0 for N ~_ 2 only required the consideration of functions e w ( ~ ) that are i~d~p~d~t of ~, in which ca~e F~I~(~) - 0, they can be reproduced v e r b a t i m for N -- 1, thus showing that U -I -- 0~

and the proof is complete.

8.8.

m

I D E N T I F I C A T I O N OF A T W O - D I M E N S I O N A L VARIATIONAL PROBLEM SATISFIED BY THE LEADING TERM

It has just been shown (Thin. 8.7-1) that the asymptotic expansion of the scaled unknown is of the form u(e) - u ~ + eu I § According to the Ansatz of the method of formal asymptotic expansions (Sect. 8.6), there thus remains to continue the cancellation of the factors of the successive powers of e in the variational equations of problem 7)(e; ft) until the leading term u ~ can be fully identified, as the solutions of an a d hoc variational problem. In this direction, the following result, due to Miara [1998, Thin. 2], constitutes the key step. A w o r d of caution. The next theorem only states (in the form of a variational problem) a necessary condition that the leading term should satisfy. While there are cases (studied in Chap. 9) where this condition is also sufficient, i.e.,where this theorem also constitutes the final stage of the application of the method of formal asymptotic expansion, there are cases (studied in Chap. 10) where additional stages (which require considerable efforts!) are needed to complete the induction, m T h e o r e m 8.8-t. Assume that the scaled unknown u(c) = (u,(~))

satis~ing problem P(s; ft) (Thin. 8.4-1) admits a formal asymptotic ezpansion of the form + e2u 2 +-.. , with ~0 e w ( ~ ) and ~ , u 2 e W 1'4 (~). u(e) - u ~ + e u I

Sect. 8.8]

A two-dimensional problem satisfied by the leading term

425

Then in order that no restriction be put on the applied forces and that the linearization trick be satisfied (Sect. 8.6), the components of the applied forces must be of the form

fi, e(Xe ) -- fi, O(x )

for all

hi, e(xe) - ehi, l(x)

for all

x e : 7rex E ~e

where the functions fi, O E L2(~) and h i'1 E pendent of e.

L2(r+ u r_) are inde-

This being the case, the leading term u ~ is independent of the transverse variable x3 and r := ( r 89f~t u~ dxs satisfies the following two-dimensional variational problem:

~0 e W(w)"-- {n e wl'4(w); n -- 0 on 7o},

f a ,~.~-E~ll~Fallf3 o o (r/) C'd dy - f . p"~ fo~ ~n n - ( ~ )

e W(~),

where (recall that a mn -- a m . an) 9

Eo Fo

1

0

1

_ m n ,,O

~.~{

0

o

o

r/all/3 : - c9/~77a- r"a~rkr - ba/~rl3, r/sll/3 "= O/3r/s + b~rl~, aaf ~~ : :

pi, O :=

4A# aa~aar + 2#(aaaaf~r + a a r a ~ ) , A+2#

f

~i, 1 + hi,_ 1 and h~ t "- h ~'"t (', + 1 ) . fi, Odxs +,o+ 1

9

426

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

[Ch. 8

Pro@ The proof comprises three parts. (i) To begin with, we remark that the conclusions of part (iv) of the proof of Thm. 8.7-1 are valid for any N >_ 0 and under the sole assumption that u(s) can be expanded as u(e) - u - N + . . . , with u - N E W(f~). Letting N - 0, we thus infer that 03u ~ - 0 in f~ and that

r176 2

1

u ~ dxa e W ( w ) : = { r / e Wl'4(w); rl - 0 on 70},

and also that (recall that the functions Eq,~ and ~q,~(v) are by definition the factors of e q in the formal exp~ansions"of the functions EillJ(e; u(s)) and FiltJ(e; u(e), v) defined in Tam. 8.4-1). E/~Ij = 0 for all integers q < - 1 , F/~Ij(v) - 0 for all integers q < - 2 and all v E W(f~), and, finally, that we must let

fi,-2

__

0 and h i'-1 - O .

(ii) Our next try is thus f i ( ~ ) __

l fi,-1 a n d h i ( e ) - h i'O

where it is understood as in the proof of Thm. 8.7-1 that each function ]i,r E L2(f~) and each function h i'r+l E L2(r+ u r_), r >_ -1, appearing here and subsequently is independent of ~; likewise, we again let

Lr(v) . - f f fi, rviv/-adx + f r

+ur_

h i,r+l v v ddr, r >_ - 1 .

The cancellation of the coefficient of e-1 in the variational equations of problem "P(e; f~) (Thm. 8.4-1) then yields the equations (the functions AiJkt(O) are defined in Thm. 8.5-2):

il]j ffz Aijkl(o)EO[ll F-l(v)~/-ddx - L-l(v)

Sect. 8.8]

A two-dimensional problem satisfied by the leading term

427

for all v E W ( ~ ) , where Eoa

1

o

=

Eoa

E~ F

~ilt3

113 --

+

1 , (0)

mn 0

0

2(.Ual13 + U31la -4,(o)

0

11o .11 ) ,

+

amnu 0

u(O)

~II~ nil3)'

l amnu(Oml u(O)

- "~3[13A-~

13 ,,113'

= 0,

1 (Oava + a mn o

03Vn),

and (the functions riP~0 are defined in Thm. 8.5-1) 0 o _ pp, 0~,o and u (~ t ~.p, 0 0 U~ll~ := OaUm - ~ m - p roll3 "- 0 3 u ~ - rm3U p, The special notation u~l13 (which thus replaces the notation uOII 3 used in the proof of Thin. 8.7-1) emphasizes that, by contrast with the functions u~ which only depend on u ~ -(u~ the functions u(~

also depend on u 1 - ( u 1) (recall that u(m~ is by definition the

coefficient of s o in the formal asymptotic expansion of Umll3(e)). For this reason, the occurrence of the functions U(m~ implies that the formal asymptotic expansion of u(e) be "at least" of the form u(~)

-

u ~ + eu

1 +....

The expressions of the functions F / ~ ) ( v ) i m p l y that L - Z ( v ) - 0 for all v = W(12) that are i n d e p e n d e n t of z3. Hence we must let / i , - 1 _ 0 and h i'O - 0 (first requirement), so that we are left with the equations v/adz = 0

for all v = (vi) e W ( f l ) . When the functions F / ~ (v) are replaced -iby their expressions given supra, the integrand in the above integral takes the form (wrO3vr + w3Osv3) for ad hoc functions w i E L4/3(~). Then Thm. 3.4-1 shows that the functions w r and w 3 vanish

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

428

[Ch. 8

in fl, i.e., that ()~aa~E~ ~ + ()~ + 2#)E~

a

+2pE~ 3 (a ar + aaaa/3ru~ (Aaaf3E~

-4-()~ + 2p)E~

-- 0 in ~,

(o)

+ ~3113'

+2paa~E~

-Oinfl.

One obvious solution to this system of three equations is E~ 3 - 0 and Aaa/3E~

+ (A + 2p)E~ 3 = 0 in f~,

but there might be other solutions to this nonlinear system. Denoting by [... ]tin the linear part with respect to (any component of) u ~ or u 1 in the expression [... 1 and using the notations of the linear case (Sect. 3.4), we have

]lin ~l13J - e~ 2lz~E 0 ]lin _ X,,a/3o0 E

[

+

+

J 3113J

o as the coefficients of e ~ in by definition of the functions E/~I3 and eill3

the formal expansions of the functions Eilla(e; u(e)) and ei[[3(e; U(e)), the latter being precisely the linear parts in the former! Since it was found in the linear case (see step (ii) in Sect. 3.4) that e~ - 0 and e3113 0 = - A +)~2 # aagJeall~ 0 in f~, the linearization trick (second requirement) suggests that we only retain the "obvious" solution found above (as shown by CoUard [1999], this plausible argument can be made entirely rigorous; cf. Ex. 8.4). (iii) Our next try is thus

fi(e ) _ fi, O and hi(e) - eh i'l. The cancellation of the coefficient of e ~ in the variational equations of problem 7~(e; ~) then leads to the equations (two terms are needed here from the expansions of the functions AiJkl(e)v/-g(e); cf. Thin. 8.5-2): L

1 -1 AiJkl(O){E~lliFi~lj(v ) + EklItF/II j (v)}v/-d dx

+ ffl Bijkl'l EklliF/llj 0 -1 (v)dx - LO (v)

A two-dimensional problem satisfied by the leading term

Sect. 8.8]

429

for a11 v C W(K~), where the functions Ei~]j and F/~lj(v ) are defined by means of the formal expansions

0 + ~E~ IJ + . - . ~ ~llj(~; u(e)) - E~ltj 1 F~llj(~; u(e), v) - ~ ~ ) ( ~ )

0 + F~jlj(v)+....

Note that, while the functions E ~ F'7'1"()2113 "v'' and F~ (v) depend only on u ~ and u 1, the functions E/~lj depend also on u 2 (but not on u3; each term involving u 3 vanishes because it contains some derivative Oau~ as a factor). For this reason the formal asymptotic expansion of u(e) must be "at least" of the form 2 +....

q--O

In particular then, we must have

ff Aijkt(O)E~

dz -- L~

for all v E W(f~) that are independent of x3 since F~(v) -- 0 for "1" such functions; equivalently, after performing the usual identification, we must have

for all r / e W(w) - { r / e Wl'4(w); r / - 0 on ")'0}. Using the expressions of the functions Aijkl(O) and the relations satisfied by the functions E/~I3 (see part (ii)), we are left with

:

f.

()~aaf3a~r +

p(aaO.a#r+ aara#O.)) EallrFallf~(~l)~ 0 0 dx

4- ff~ (4paaaE~176 +

/o

()~aarEOll r + (X +

12foaa~E~176

4-AaaBE~176

) x/adx

2#)E3113 o ) F~)lla(r/)~dx dx -

L~

430

[Ch. 8

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

for all rl E W(w), where aO~f~ o-.r .__

4A# aa~a,7r + 2p(aaCra~.r + aar af3O.). A+2p

Since u ~ E W ( f t ) is independent of x3, it may be identified with a function ~0 C W(w). Consequently, the functions EOll~ = ~(~~ 1 o ) e L2(~ ) , , + U~lla~+ ~mnum10laUnllf3

F211~('~)=

1 ~('7,,11~ + '7~11,~+

amn

0 0 {",,,11,~'7,,11~ + ",,I1~'7,,,11o})e

L2

(~),

which are thus also independent of x3, may be likewise identified with functions (denoted for convenience by the same symbols)" Eo II~ = ~(~oll~ 1 0 + ~ll~ + ~_mn.o ~0 ~ll~-It~)

FOal

1

amn

0

e L 2(~1, 0

L2

where r/ail/9 - O~rla -r~D~Ta --ba~9~73 and ~73[I/3-- 0~9z}3-{-b~r/~ for all ~ - (r/~) E W(w). The last variational problem is thus indeed two-dimensional, m

The functions a a~r found in Thm. 8.8-1 are the contravariant components of the scaled two-dimensional elasticity tensor of the shell, already encountered in the linear theory (see, e.g., Sect.

3.4).

EXERCISES

8.1. The three-dimensional energy J in Cartesian coordinates associated with a St Venant-Kirchhoff material is defined by (the notations are those of Sects. 8.1 and 8.2)" 1

Ezercises

431

Show that there exist constants a > 0 and/3 ~ I~ such that -

'Ca) +

for all ~ e W ( ~ ) - {~ = (~3i) e W~'4(h); ~ = 0 on r 0 ) . Remark. The energy .] is thus coercive on the space W ( ~ ) . It cart be shown, however, that it is not weakly lower semi-continuous on W ( ~ ) ; cf. Ball & Murat [1984], Raoult [1986], Dacorogna [1989], Le Dret & Raoult [1995a]. 8.2. (1) Using the notations introduced at the beginning of Sect. 8.2, show that the variational equations in Cartesian coordinates of Sect. 8.1 may be equivalently rewritten as

O) d~ - /f /i~)id~ + f hivi aT, 1

where

(2) Using the notations and definitions of Thms. 8.2-1 and 8.2-3, show directly, i.e., without resorting to the functionals .] and J found in these theorems, that

~) d~ - f a AiJkIEkllt(u)Fillj(u' v ) v / g dx.

8.3. Show that the boundary value problem of three-dimensional nonlinear elasticity in curvilinear coordinates (Thm. 8.2-4), viz.,

-(~/J + crkJg/~u~llk)llj -- A in KZ, ui = 0 on to, (aij + ahJgitulllk)nj -- hi on r l , where a ij - AiJklEkllt(u), can be directly derived from its Cartesian counterpart (Sect. 8.1), viz.,

~i -

0 on to,

432

Asymptotic analysis of nonlinearly elastic shells: Preliminaries

[Ch. 8

where a ~j - .4iJkZ/~kZ(/L) ("directly" means without recourse to the variational equations, as in Thm. 8.2-4). 8.4. It was observed in part (ii) of the proof of Thm. 8.8-1 that an obvious solution to the nonlinear system of equations: (Aaaf~E~

+ (A -4- 2p)E~

3

-4-2pEa~ 3 (a ar A-- a atra/3ruO/3tia) - 0 in [2, (o)

+2paa~EOll 3u311 ~0 -- 0 in [2 is

_a~O E~ s -- 0 and ~~,~, ~ail~ + ()~ + 2p)EOIi 3 - - 0 in ~.

The objective of this problem is to find all the other solutions. (1) Show that another solution is u(~l3 - 0 a n d

U~l~)3 - - 1 .

(2) Show that all the remaining solutions are of the form u(a~I3 -- (aa/3 + U~

(o)

o

~ and "3113 - u3iiaw

- 1,

where the functions w a depend only on the functions u~ Remark. These results are due to Collard [1999].

CHAPTER 9 NONLINEARLY

ELASTIC

MEMBRANE

SHELLS

INTRODUCTION

The purpose of this chapter is to identify and to mathematically justify the two-dimensional equations of nonlinearly elastic "membrane" shells. These equations are of two kinds, depending on whether they are obtained through the method of formal asymptotic expansions or by means of a convergence theorem. We begin with the formal approach, which is due to B. Miara. Given a surface S = O(w) and a displacement field yia i of S with smooth enough covariant components r/i : ~ --~ 1~, let aao(r/) denote the covariant components of the metric tensor of the associated deformed surface (0 + ~Tiai)(-~). A nonlinearly elastic shell with middle surface S subjected to a boundary condition of place along a portion of its lateral face with 0(3:0) as its middle curve, where 70 C 7, is a nonlinearly elastic "membrane" shell if the manifold ~ 0 ( w ) = { r / = (Yi) e w l ' 4 ( w ) ; r / = 0 on 70, aaB(rl)-aaB = 0 in w}

reduces to {0} (Sect. 9.1). This means that 0 is the only displacement field rlia i of the surface S with covariant components ~i in W1,4(w) that is admissible and ineztensional, i.e., that vanishes along the curve 0(70) and leaves invariant the metric of S. This definition is motivated by the crucial observation that the induction begun in the previous chapter ends when ~ 0 ( w ) = {0}. The conclusions reached in Thm. 8.8-1 can then be reformulated as follows in this case (Thm. 9.2-1): Assume that ~ 0 ( w ) -- {0}. Then the contravariant components of the applied body forces must be of the form

/i'e(Xe)

: fi'0(X) for all x' -- 7r'x E f~',

where the functions ]i,0 are independent of e (for simplicity, we assume in this introduction that there are no surface forces), the

Nonlinearly elastic membrane shells

434

[Ch. 9

leading term u ~ 9-~ --+ I~3 o/ the formal asymptotic expansion of the scaled unknown is independent of the transverse variable, and r ~ f~_~ u ~ dz3 satisfies the following (scaled) two-dimensional variational problem o/ a nonlinearly elastic "membrane" shell: r

e w~(~)

- { ~ e w ~ , 4 ( ~ ) ; ~ = o oil ~0},

aaf3a'rGa'r(~o)(Gla/3(~~ ~/~dy - ~ pi'O~Ti~rady for all r / - (r/i) C WM(w), where, for any ~, r/E w l ' 4 ( 0 g ) , 1

1

G o ~ ( o ) = ~ ( a . ~ ( O ) - a.~) = ~(U-il, + ~,li- + I

am"~mll"~nll')'

1

aO~f~ O'T _

f,

p,, o _

4)~# aa~ aO.T + 2#(aaCraf3r + aar a/3O.), )~+2#

1

/,, o dza.

The functions Gaf3(r/) and a a/3~r are respectively the covariant components of the change of metric tensor associated with a displacement field 77iai of the middle surface S and the contravariant components of the (scaled) two-dimensional elasticity tensor o/ the shell. These equations also express that ~0 is a stationary point o / a certain functional over the space WM(W), so that particular solutions may be obtained by solving a minimization problem (Thm. 9.3-1), written here directly in its "de-scaled" version (Thm. 9.4-1): The vector field ~e = ( ~ ) formed by the covariant components of the limit displacement field ~ a i of the middle surface S satisfies" ~e e WM(W) and j ~ ( ~ e ) =

inf j~f(r/), n~WM(~)

where the two-dimensional energy jeM of a nonlinearly elastic membrane shell is defined by a a~Crr'e(a,Tr (17) - aar)(aa~(~) - aa~)V~ dy f pi, e~Tiv/-ddy,

Introduction

435

where 4 A e p ~ aa~SaSt" + 2/.te (aaO-alSr + aar a/SO-),

As + 2p ~ p,,e =

f,,e dx~. e

The functions a a~vr are the contravariant components of the twodimensional elasticity tensor of the shell, Ae and #e are the Lamfi constants of the material constituting the shell, and the functions fi, are the contravariant components of the body force density applied to the shell. The stored energy function of a nonlinearly elastic membrane shell is thus remarkably simple: It is a quadratic and positive definite expression in terms of the ezact difference between the metric tensor of the deformed middle surface and that of the undeformed one. Incidentally, this shows that the equations of the linear theory of "membrane" shells are immediately recovered (at least formally) under linearization of the nonlinear equations. We also briefly discuss in Sect. 9.4 approaches that could lead to an existence result for the above minimization problem or for the associated boundary value problem (Thin. 9.4-2). We conclude this chapter by reviewing in Sect. 9.5 a justification of yet another two-dimensional "membrane" shell theory, this time by means of a convergence theorem, the first of its kind for shells. More specifically, another two-dimensional minimization problem for a nonlinearly elastic shell has been derived from nonlinear threedimensional elasticity by H. Le Dret and A. Raoult for a realistic class of hyperelastic materials. Using F-convergence theory, they have shown that the minimizing deformations of the three-dimensional energies, once appropriately scaled over a fixed domain f~ C I~3, weakly converge in the space Wl,V(f~) as the thickness of the shell approaches zero (cf. Thm. 9.5-1; the exponent p > 1 is "governed" by the hyperelastic material considered). The limit deformation found in this fashion is independent of the transverse variable and minimizes a limit energy obtained by computing the F-limit of the three-dimensional energies; hence the existence of a minimizer of this limit energy is de facto established.

Nonlinearly elastic membrane shells

436

[Ch. 9

The limit stored energy function is again that of a nonlinearly elastic "membrane" shell, in the sense that it contains only first derivatives of the unknown deformation. For a St Venant-Kirchhoff material, it does not coincide, however, with the energy found via the method of formal asymptotic expansions, save when the singular values of the limit deformation gradients belong to a specific subset of the plane. For this reason, it does not always reduce under linearization to the linear theory of "membrane" shells. The origin of such differences may lie in that the latter approach models shells made with "soft" elastic materials (like the sails of a sailboat or a balloon), while the former models shells made with "rigid" elastic materials (like the hull of a ship or the roof of the Hong Kong Convention and Exhibition Centre). But this affirmation is yet to be substantiated. 9.1.

N O N L I N E A R L Y E L A S T I C M E M B R A N E SHELLS: DEFINITION, EXAMPLES, AND ASSUMPTIONS ON THE DATA

The analysis of Chap. 8 culminated in Thm. 8.8-1, where it was shown that the leading term u ~ of the formal asymptotic expansion of the scaled unknown u(e) is independent of x a and that ~0 := 1 f_l 1 u 0 dxs satisfies:

r = (r

e

- o on 7o}

e

and f~

aaf~arEOl[ r alif3(n)v/-ddy pZ'~ F~ f~ "

for all r / = (r/i) E W(w), where

EOll~ "-

1(C~

+ C llo +

amn o

o C, ll Cnll )"

An inspection of the functions E~ ~ appearing in the left-hand side of the variational equations thus immediately reveals that two fundamentally distinct situations must be considered, depending on whether there are non-zero fields r/ = (r/i) in the space W(w) that satisfy r/all~ + ~lla + amnr/mllar/n[lD - 0 in w.

Sect. 9 . 1 ]

Definition, ezamples, and assumptions on the data

437

If there are no such fields, the induction is terminated (this situation is studied in this chapter), while the induction may be continued if there are such fields (see Sect. 10.1). In this direction, the first task consists in recognizing in the functions E all~ ~ (half of) the differences between the covariant components of the metric tensor of the "deformed" surface (0 + ~~ and those of the metric tensor of the "undeformed" surface S = 8(~) and then in showing that the functions F~ are simply G~teaux derivatives at ~0 of these differences. Together, these expressions will in turn provide an illuminating interpretation of the variational problem satisfied by ~0 (Thm. 9.2-1) (the definitions of the covariant and mixed components baf~ and b~ of the curvature tensor and the Christoffel symbols I~f~ of S appearing in the next theorem are recalled in Sect. 8.5). T h e o r e m 9.1-1. Let w be a domain in ~2 and let 8 E g2(~; I~3) be an injective mapping such that the two vectors aa = Oa8 are final A a 2 early independent at all points of-~, let a3 - [al A a2[' and let the vectors a i be defined by a i . a j - ~ . Given a displacement field ~Tiai of the surface S 8(-~) with smooth enough covariant components Yi " -w -+ R, let the covariant components of the c h a n g e of m e t r i c t e n s o r associated with this displacement field be defined by 1

a . ~ ( n ) := ~ (a.~(n) - aa~) , where aa~ and aaf3 ( y ) are the covariant components of the metric

of

(O + 1

-

i(n-lJ

+ n il- + m n ll-n it ),

r/allf3 := 0/3~7a - F ~af}Tla.- baDr]3 and ~7311f3:= Ofjr/3 + b~?a. The Gdteaux derivatives of each function Gaf3" W 1' 4(w) ~ L2(w) are given by 1

am n

Nonlinearly elastic membrane shells

438

for all ~, r/ C W~'4(w)

9

[Ch. 9

In particular then, the functions E ~

all~

and

F~ appearing in the variational problem found in Thin. 8.8-1 are also given by

E~

= a a # ( r ~ and F~

= a~af3(r176

Proof. Let 0 "--yia'. By definition,

a,e(n) - (a, + o~,)). (ae + oe#) = a,~+o~O.a,~ +O,~O'a~+O,,O'O~O. By the formulas of Gaufl and Weingarten (Thm. 2.3-1), OaO - ~ l l a a ~ + r/311~a3, Since a i . a a - ~ia and a m . a n - a ran, it thus follows that

aa~(rl) - aa# -- r/all# + ~Z311a+ amn~mlla~nll~" Hence E~ - Ga/s(r176 That F~ - G'a#(r176 results from the way derivatives of continuous linear and bilinear mappings are computed (see, e.g., Vol. I, Sect. 1.2). II

Remarks. (1) The functions ~?illft may be also expressed in terms of the "two-dimensional" covariant derivatives rlil~ of the vector field 0 = rlia i (Thin. 2.3-1) as ~llz3 - ~1~ - ba[3~73 and ~7311~- r/31~l - b~r/~. The double bars used in the functions r/i[]f3 remind that they are restrictions for x3 = 0 of "three-dimensional" covariant derivatives

(Sect. 1.4). (2) The components Gaf3(r/) of the change of metric tensor are the restrictions for x~ - 0 of the "three-dimensional" strains E s ~llj(v~) with r / : = velz3=0. This was to be expected in view of their respective significances (Thms. 8.2-2 and 9.1-1). i

Sect. 9 . 1 ]

Definition, ezamples, and assumptions on the data

439

In this chapter, we consider the case where the only field ~1 = (71i) in the space W ( w ) - { r / E W 1' 4(w); r / - 0 in w} that satisfies 7/all~ -f- ~?/31la-4- amn~lmlta~Tnll/3 -- aa#(~l) -- aa# = 0 in w

is r/ = 0. This assumption, combined with Thin. 8.8-1, then leads to the following fundamental definition: Let w be a domain in I~2 with b o u n d a r y 7 and let 0 E g2(~; i~3) be an injective mapping such that the two vectors 0a0 are linearly independent at all points of ~. A nonlinearly elastic shell with middle surface S = 0(~) is called a n o n l i n e a r l y e l a s t i c m e m b r a n e shell if the following two conditions are simultaneously satisfied: (i) The shell is subjected to a boundary condition of place along a portion of its lateral face with 0(70) as its middle curve, where the subset 70 C 7 satisfies length 70 > 0. (ii) Define the manifold: := {n

-

c

,1 a,

z(n) -

0 o= a, a -

o i=

Then = {o).

A displacement field ~Tia i of the middle surface S is an i n e x t e n d i s p l a c e m e n t of S if aa~(~/) - aa~ = 0 in w. These relations imply t h a t the surfaces S - O(~) and (O + ~iai)(-~) are i s o m e t r i c , i.e., t h a t their metrics are the same (in particular then, the lengths of curves are the same; cf. Sect. 2.1). A displacement field ~Tia i of the middle surface S is a d m i s s i b l e if it satisfies ad hoc b o u n d a r y conditions along the curve 8(70), in the present case "boundary conditions of simple support", expressed by means of the b o u n d a r y conditions ~ / - 0 on 7o on the associated field 17 = (~/i) (these b o u n d a r y conditions are interpreted later; cf. Sect. 9.4). The assumption ~ t 0 ( w ) -- {0} thus expresses that the only admissible (i.e., such t h a t r/i - 0 on 3'0) inextensional displacement yia i of the middle surface S with covariant components Yi in the space W l'4(w) is zero. sional

440

Nonlinearly elastic membrane shells

[Ch. 9

e(z0• I-a, a])

Fig. 9.1-1: A nonlinearly elastic membrane shell. A shell whose middle surface S = 0(~) is a portion of a cylinder and which is subjected to a boundary condition of place (i.e., of vanishing displacement field) along a portion (darkened on the figure) of its lateral face whose middle curve 0(70 ) contains the two "end-curves" of S provides an instance of a nonlinearly elastic membrane shell, i.e., one for which the manifold M O ( W ) = { ~ = (17i) E W l' 4(O./); 71 = 0 o n 7 o , a a o ( r / ) - a a o = 0 i n w }

reduces to {0}; cf. Ex. 9.1.

E z a m p l e s of nonlinearly elastic m e m b r a n e shells are shown on

Figs. 9.1-1 a n d 9.1-2 a n d analyzed in Exs. 9.1 a n d 9.2.

A w o r d o f c a u t i o n . T h e definition of a nordinearly elastic memb r a n e shell depends only on the subset of the lateral face where the sheU is subjected to a b o u n d a r y condition of place (via the set 70) a n d on the geometry of the middle surface of the sheU (via its two fundam e n t a l forms a n d Christoffel symbols, which a p p e a r in the functions ~i[l~); see Ex. 9.3. m

A n o t h e r w o r d o f c a u t i o n . A l t h o u g h the above definition is strongly suggested by the a s y m p t o t i c analysis, it is a d m i t t e d l y perfectible, as it leaves aside nonlinearly elastic shells t h a t should also be d e e m e d " m e m b r a n e " ones.

Sect. 9 . 1 ]

Definition, ezamples, and assumptions on the data

441

r

Fig. 9.1-2: Another ezample of a nonlinearly elastic membrane shell. Consider a plate subjected to a boundary condition of place on a portion of its lateral face whose middle line 70 has the following property: There exists (at least) one direction such that the intersection of ~ with any line parallel to this direction is a finite union of segments whose end-points belong to 70 (this is thus the case if 7o = 7)- Then such a plate is a nonlinearly elastic membrane shell; el. Ex. 9.2. By contrast, such a plate is always modeled as a flex~al shell (even if 70 = 7) when it is viewed as a linearly elastic body! See Fig. 6.1-3.

C o n s i d e r for i n s t a n c e a shell whose m i d d l e surface is a half-sphere, s u b j e c t e d to a b o u n d a r y c o n d i t i o n of place along its entire l a t e r a l face (i.e., 70 = 7). T h e n :~40(w) ~ {0}, since s y m m e t r i e s w i t h r e s p e c t to planes o r t h o g o n a l to the axis of r e v o l u t i o n p r o d u c e a family of continuously varying isometric surfaces (O + ~Tiai)(-w) w i t h rl - (yi) e W l ' ~ 1 7 6 a n d rl r 0. Hence such a n o n l i n e a r l y elastic shell is not a " m e m b r a n e " one a c c o r d i n g to the above definition. Yet it is n e i t h e r a "flexural" one according to the definition given in Sect. 10.2, as it seems plausible t h a t the m a n i f o l d ~'t~,(w) i n t r o d u c e d in ibid. contains only two elements (the covariant c o m p o n e n t s of t h e a d m i s s i b l e i n e x t e n s i o n a l d i s p l a c e m e n t s in ~4~,(w) are t h e n r e q u i r e d to be in W2'4(w); see a g a i n Sect. 10.2). As h i n t e d by this e x a m p l e , w h e t h e r or not a m a n i f o l d of i n e x t e n s i o n a l d i s p l a c e m e n t s reduces to a finite set or not critically d e p e n d s on the smoothness allowed on the admissible inextensional displacements.

442

Nonlinearly elastic membrane shells

[Ch. 9

This challenging question is related to that of the rigidity of surfaces, a classical problem in differential geometry: A compact surface "without boundary" is rigid if any other such surface in IR3 with the same metric differs from it by a rigid deformation, i.e., a mapping of the form x E I~3 --~ a + Q o z , where a E I~3 and Q is an orthogonal matrix of order three; again, the allowed smoothness on the surfaces play a critical r61e. See, e.g., Pogorelov [1956], Nirenberg [1962], Klingenberg [1973, Thin. 6.2.8], Spivak [1975, Vol. V, Chap. 12], Berger & Gostiaux [1992, Thin. 11.14.1]. The same question can also be viewed as one about the existence of everted states under vanishing applied forces. For details about such eversion problems for shells (examples are given in Vol. I, Figs. 5.8-1 and 5.8-2), see in particular Srubshchik [1968, 1972, 1980], Vorovich [1969], Mel'nik & Srubshchik [1973], Antman [1979], PodioGuidugli, Rosati, Schiaffino & Valente [1989], Szeri [1990], Geymonat & L~ger [1994], Antman [1995, pp. 501-503], Antman & Srubshchik

[1998].

m

Since the formal asymptotic analysis ends with Thm. 8.8-1 when ~vt0(w) = {0), we are naturally led to make the following a s s u m p t i o n s on t h e d a t a for a family of nonlinearly elastic membrane shells, with each having the same middle surface S = 0(~) and with each subjected to a boundary condition of place along a portion of its lateral face having the same set 0(70) as its middle curve, as their thickness 2e approaches zero: We require that the Lamd constants and the applied body and surface force densities be such that

)~e = A and #e = #, fi'e(xe) = fi'O(x) for all x e = 7rex E f~',

hi'e(z e) - ehi'l(x)

for all

x' - 7re~ C I'~_ U r ~ ,

where the constants )~ > 0 and # > 0 and the functions fi, o E L2(f~) and h i'1 C L2(r+ U r _ ) are independent of e (Fig. 3.2-1 recapitulates the definitions of the sets f~e, f~, r ~ , r + , r e_, and r _ ) .

Note that the same limit two-dimensional equations are evidently obtained if the following more general a s s u m p t i o n s on t h e d a t a

Sect. 9.2]

The two.dimensional equations as a variational problem

443

are made: ,ke = ~t)~ fi'~(x') - etfi'~ ") -

and for all for an

pe = 6tp, x ~ - 7r'x C f~', -

u r'_

where the constants .k > 0 and p > 0 and the functions fi,0 E L2(f~) and h i' 1 C L 2 (I~+ (2r_) are again independent of 6 and t is an arbitrary real number. Besides, the analysis of Chap. 8 (see in particular Thm. 8.8-1) shows that these assumptions on the data are the only ones possible for nonlinearly elastic membrane shells. 9.2.

THE TWO-DIMENSIONAL VARIATIONAL PROBLEM

E Q U A T I O N S AS A

We know from Thm. 8.8-1 that the leading term u ~ of the formal asymptotic expansion of the scaled unknown u(6) is independent of the transverse variable x3 and that, once identified with a function ~0 of two variables, it satisfies a two-dimensional variational problem. When the manifold 2rio(w) reduces to {0} (Sect. 9.1), no inconsistency arises in the formulation of this problem, and thus the induction stops here. We also saw in Thin. 9.1-1 that the functions E~ ~ and F~ occurring in the formulation of this problem have more illuminating expressions than those found in Thm. 8.8-1; as a result, these new expressions shed a new light on the understanding of this variational problem, henceforth denoted 79M(W). The equivalent boundary value problem is given later; cf. Thm. 9.4-2. The following result, which is an immediate corollary to Thms. 8.8-1 and 9.1-1, is due to Miara [1998]. Notice that a new notation, viz., WM(W), is used from now on in this chapter for the space heretofore denoted W(w). T h e o r e m 9.2-1. Consider a family of nonlinearly elastic membrane shells according to the definition of Sect. 9.1, with thickness 2~ > O, with each having the same middle surface S = O(-~) and with each satisfying a boundary condition of place along a portion of its lateral face having the same set 8(70) as its middle curve, and let the assumptions on the data be as in Sect. 9.1. Finally, assume that 0

C3( ; R3).

Nonlinearly elastic membrane shells

444

[Ch. 9

Then the leading term u ~ 9-~ -+ IR3 of the formal asymptotic expansion of the scaled unknown u(e) is independent of the transverse variable and ~o .-'- 1_2s u~ dx3 satisfies the following scaled t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m ~M(W) of a n o n l i n e a r l y elastic m e m b r a n e shell:

~0 e WM(W)"-- {r/e Wt'4(w); r/-- 0 on 70},

~ aaf3arGar('~(G~;3(,~

- L pi'~

dy

fo~ ~ n . = (,i) e W ~ ( ~ ) .

where,/or any r ~/ e Wt'4(w) (the functions aa~3(r/) are defined in Thm. 9.1-1),

1 1

= ~(~il~ + ,7~lt,~ + a"%~ll,~'7-1it3), ,

1

aat3(r

-

~('7ol1~ + '7~li,~ + a'"{c:,~lio'7,~li~ + c:,.li~'7,.ilo}),

r/all~ "= O~r/a aaO~r~. .=

F~t3~/~-

ba/3'q3

and ~3il/3 : - - 0/3'/'/3 + b~r/o-,

4X# aa~ a,~r + 2#(aa,~aOr + aa ~.aoa) ' $+2#

f , .o ._.

.

. ~i, 1 /,,o dz3 + h~ z + h ''z and ,o+ := h ~'" 1 (., +1),

1

and Ga~(~ I ) E s 1 4(w); L2(w)) denotes the Fr~chet derivative at E Wl'4(w) of each mapping Ga[3" w l ' 4 ( w ) -+ L2(w). II

Notice the analogy between the two-dimensional variational problem PM(W) and the variational problem of three-dimensional nonlinear elasticity we started from (Thm. 8.2-3).

Sect. 9.3]

9.3.

The two-dimensional equations as a minimization problem

THE TWO-DIMENSIONAL EQUATIONS MINIMIZATION PROBLEM

445

AS A

As noted by Miara [1998], the aforementioned analogy can be pursued further: First, the variational equations found in the twodimensional and three-dimensional problems simply express in each case that the Ggteaux derivatives of an ad hoc functional vanish; second, the integrand in the functional is in each case (apart from its linear term accounting for the applied forces) a quadratic and positive definite expression (via an elasticity tensor) in terms of a change o]

metric tensor. These crucial observations in turn allow to recast the two-dimensional variational problem 79M(W) as a minimization problem, which now exhibits a remarkable simplicity. In this problem lies the apex of the application of the method of formal asymptotic expansions to nonlinearly elastic membrane shells. T h e o r e m 9.3-1. Given a nonlinearly elastic membrane shell according to the definition given in Sect. 9.1, let the space WM(W) and the functional jM " WM(W) -+ I~ be defined by WM(W)

"-- { ~ -- (~7i) e W I ' 4 ( W ) ; ~ -- 0 o n ' ~ 0 } ,

1~ a a ~ r (aa.v(n) -

j M ( n ) "-- ~

a~r)(aa~(l?) - a a ~ ) v ~ d y -- f~ Pi' ~

dY'

where the functions aa#(17) are defined in Thin. 9.1-1 and the functions a a#~r and pi, 0 are defined in Thin. 9.2-1. Then the functional jM is differentiable over the space Wl'4(w), hence over WM(W), and r C WM(~) is a solution to the variational problem ~DM(W) Of Thm. 9.2-1 i] and only if it is a stationary point of the functional jM over the space WM(w), i.e., it satisfies j~M(~~ -- O. Particular solutions to problem 79M(W) are thus obtained by solving the minimization problem: Find ~ such that r E WM(W) and j M ( r

inf

neWM(.~)

jM(rl).

Nonlinearly elastic membrane shells

446

[Ch. 9

Proof. Since

jM(O) - ~l ~ a a f 3 t r r a~(O)a,,~(O)4"ddy-

f pt'~ "

where 1 G af3 Cvl ) -- "~( aaf~ ( vl ) -- aaf3 )

1 = ~(rh~ll~ + rl~lla + a'~n'q~ll,~r/,~ll~), an argument similar to that used in the proof of Thm. 8.2-3 shows that j M is differentiable over Wl,4(w) and that its G~teaux derivatives j ~ ( ~ ) y are given by

jtM(~) . -- ~aaf~a'r(~o.r(~)((~tafl(~),q)vfady- fwpi,~ for all ~, y E Wl'4(w), where 1

a',(r

= ~(~11, + ~,ll~ + a~"{r

+ i-li,~ll~})"

The variational equations satisfied by ~0 E WM(w) (Thm. 9.2-1) thus coincide with the equations

j~(r

_ 0 fo~ ~n ~ e w ~ ( ~ ) ,

which are themselves equivalent to the equation j~(~0) _ 0. That it makes sense to consider the above minimization problem stems from the observation that inf JM(~) >--OO, n~WM(~) an inequality itself a consequence of the coerciveness of the functional over the space WM(w) (Ex. 9.4). The existence theory proper is otherwise fragmentary at the present time; see the discussion in the next section, i

jM

The functional j M " WM(w) --~ ]~ is called the scaled twod i m e n s i o n a l e n e r g y of a n o n l i n e a r l y elastic m e m b r a n e shell.

Sect. 9.4] 9.4.

The two-dimensional equations derived by a formal analysis

447

TWO-DIMENSIONAL EQUATIONS OF A NONLINEARLY ELASTIC MEMBRANE SHELL THE

DERIVED

BY MEANS

ASYMPTOTIC

OF A FORMAL

ANALYSIS; COMMENTARY

In order to get physically meaningful formulas, it remains to descale the components (o of the vector field ~0 that satisfies the scaled two-dimensional problems found in Thms. 9.2-1 and 9.3-1. In view of the scalings ui(~)(x) - u~(x e) for all x e - vrex e ~e made on the covariant components of the displacement (Sect. 8.4), we are naturally led to defining for each ~ > 0 the c o v a r i a n t c o m p o n e n t s ~ 9~ --4 I~ of the l i m i t d i s p l a c e m e n t field ~e ._w__4 I~3 of the middle surface S of the shell by letting (the vectors a i form the contravariant basis at each point of S): r := (o and ~ := r

i.

Remark. I realize that, ]or once, my notations ( ~ vs. ~o) are somewhat misleading! 1 A w o r d of c a u t i o n . Naturally, the fields ( ~ ) and ~e _ ~ a i must be carefully distinguished! The former is essentially a convenient mathematical "intermediary", but only the latter has physical significance. 1 Recall that fi,~ E L2(~ e) and h i'c E L2(r u r!) represent the contravariant components of the applied body and surface forces actually acting on the shell and that Ae and p~ denote the actual Lamd constants of its constituting material. We then have the following immediate corollary to Thms. 9.2-1 and 9.3-1. T h e o r e m 9.4-1. Let the assumptions be as in Thm. 9.2-1. Then the vector field ~e := ( ~ ) formed by the covariant components of the limit displacement field ~ a i of the middle surface S satisfies the following t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m 7)~(w) of a

448

Nonlinear'ly elastic membrane shells

nonlinearly

elastic m e m b r a n e

r e w.(~).=

[Ch. 9

shell:

{n e w~.4(~); n = o on ~0},

fo~ ~ n , = (~) e W u ( ~ ) , where 1 a . , ( , 7 ) "= 5 ( a . , ( ' l ) - a . , ) 1

= ~(~11~ + ~il,~ + a'~"'~-,li,~,,ll~), a'~(r

1

= ~(~oll~ + ~ll~ +

am n

{i~ll~,ii~ + ~ - t l ~ i l ~ } ) ,

r/allfj "-- Of3rla -- F~flrla -- ba~vl3 and v/31lf~"- Off'r/3 -4- b~vkr, aa~ar, e 9= p',~ . -

4)~ei~e aa/3a ~r + 21~e(aaea[3r + aara~e), A e + 2# e f

r

. . . ]',~ e ~ + h ;, ~ + h ',~ a=d h~. ~ . - h"~(., •

6

The field r _ ( ~ ) is a solution to problem 7)~(w) if and only if it is a stationary point of the functional j ~ " W M ( w ) ~ ~ defined by

jeM(~}) "= ~r f~ aa/3crr,e (a~r(~}) -- a~r)(aa~(~l) -- aa~)~fa dy -- f~ Pi' e~Tiv ~ dy"

Particular solutions to problem 7)~(w) may thus be obtained by solving the following minimization problem: Find ~e such that

~e E WM(W) and j ~ c ( r

inf j~c(r/). n~WM(.,) m

Sect. 9.4]

The two-dimensional equations derived by a formal analysis

449

We next derive the boundary value problem t h a t is (at least formally) equivalent to the variational p r o b l e m 7 ~ ( w ) found in T h m . 9.4-1. In the next theorem, (t,a) denotes the unit outer n o r m a l vector along 3' a n d 3'z := 3 ' - 3'0Theorem 9.4-2. Let the assumptions and notations be as in Whm. 9.4-1. If a solution ~e _ (i~) to the variational problem

e f aa~3~r'eGvr(,e)(G~a/3(,e)rl)v/-ddy-f pi'e~liV/-ddy for all r / :

(~i)

e

WM(60)

is smooth enough, it also satisfies the following boundary value problem: $

- ( n al3,e + n aG "aar~rlla)l~ + b~na/3'er

_ba/3(na/3, e + n~,eaars -~tl~) - (na~,e r e

~ _.._pOtg' in w,

: r ,3'' in w, ff~ = 0 on')'o,

(rta/3, e 4- n ~13' e u_ a r , 'qrll~ e ~/) ) D -- 0on71, e

na#(311avr -- 0 on 71,

where

n~,, ._ e~~,,~a~(r the functions Ga~(~e), a aoar'e, and pi, e are defined as in T h m . 9.4-1 and, for any vector field with differentiable contravariant components ~a : -~ __+ R and any tensor field with differentiable contravariant components n a[3 9 --+ R,

~~

-

o,~ ~ + r]~

~ ~na n ~

"= O~no~ + r ~ n ~ + r ~ n ~

Nonlinearly elastic membraneshells

450

[Ch. 9

Proof. For notational brevity, the dependence on e is omitted. Using Green's formula as in the proof of Thm. 4.5-1, we obtain l ~ ~na~(~Tall/3 + Y/311a)dY- - ~ ~{(na/sl/3)~?a + ba/3na~y3) + f~ v/'ana/3v/3yadT, 1_2~ V/-dna/3amn {~mlla~Tnll# +" ~nlt/3~Tmlla}dy =

f~ V/-dna/3amn~mlla~Tnll/3dy

=- f~ ~{(n~a~l~ll.)la -b~n~i311~}U~dy -

f~ ~/a{ba/3n~[3aar~rll~ + (na~311a)]~}y3 dy

+

+

}

for all (rli) e w l ' 4 ( w ) . Letting (Yi) vary first in (D(w)) 3, then in WM(W), yields the announced boundary value problem, m Each one of the three formulations found in Thms. 9.4-1 and 9.4-2 constitutes one version of the t w o - d i m e n s i o n a l e q u a t i o n s of a n o n l i n e a r l y elastic m e m b r a n e shell (the specific meaning conveyed by "membrane" is given below). 1 The functions Ga~(~/)- ~(aa~(~/)aa~) are the covariant components of the c h a n g e of m e t r i c t e n s o r associated with a displacement field yia i of the middle surface S (Thm. 9.1-1) and the functions a a~crr'e a r e the contravariant components of the t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of t h e shell. The functional j ~ 9WM(W) -+ I~ is the t w o - d i m e n s i o n a l energy, and the functional

r ~ aa~ar'e (a~r(rl)-

9/ e WM(W)-+ g

a~r)(aa~(17)- aa[3)x/ady

is the t w o - d i m e n s i o n a l s t r a i n energy, of a n o n l i n e a r l y elastic m e m b r a n e shell. Finally, the functions n a~,e are the contravariant components of the s t r e s s r e s u l t a n t t e n s o r field. The functions yal~ are instances

Sect. 9.4]

The two.dimensional equations derived by a formal analysis

451

of first-order covariant derivatives of a vector field defined by means of its contravariant components ya and the functions n af3 I~ are firstorder covariant derivatives of a tensor field defined by means of its contravariant components n af3 (such covariant derivatives have already been encountered in Thm. 4.5-1). Considered as relations with respect to the ]unctions n af3,e, the partial differential relations in w and the boundary conditions on 71 found in Thm. 9.4-2 constitute the t w o - d i m e n s i o n a l e q u a t i o n s of e q u i l i b r i u m of a n o n l i n e a r l y elastic m e m b r a n e shell. The relations n a~'~ - eaa~ar'eGaf3(~ e) constitute the t w o - d i m e n s i o n a l c o n s t i t u t i v e e q u a t i o n of a n o n l i n e a r l y elastic m e m b r a n e shell. Finally, the boundary conditions Yi - 0 on 70 express that the points of the undeformed and deformed middle surfaces 0(~) and (0 § ~iai)(-~) coincide along the curve 0(70). For this reason, they are called t w o - d i m e n s i o n a l b o u n d a r y c o n d i t i o n s of s i m p l e support. A major conclusion is thus that, without any recourse to any a priori assumption of a geometrical or of a mechanical nature, the

method of formal asymptotic expansions provides a justification of the two-dimensional equations o] a nonlinearly elastic membrane shell, in the forms found in Thin. 9.4-1. This justification by Miara [1998] constitutes a generalization to shells of the formal analysis of Fox, Raoult & Simo [1993], who likewise identified and justified the twodimensional equations of a "nonlinearly elastic planar membrane", i.e., one for which the mapping O is of the form O(yl, Y2) -- (Yl, Y2, 0) for all y -: (yl, y2) C ~ (see also Vol. II, Sect. 4.12). Further important conclusions and comments are in order about the present justification: First and foremost, the resulting shell theory is a n o n l i n e a r " m e m b r a n e ~' t h e o r y in the sense that the s t o r e d e n e r g y funct i o n of a n o n l i n e a r l y elastic m e m b r a n e shell, defined by r/-

(~7i) e Wl'4(w) -4 g aa/3~rr' e (acrr(r/)- aar)(aao(rl)- aao),

is a quadratic and positive definite expression (via the two-dimensional elasticity tensor of the shell) in terms of the change o/metric tensor, i.e., of the exact difference between the metric tensor of the deformed middle surface and that of the undeformed one.

452

Nonlinearly elastic membrane shells

[Ch. 9

Note in passing the truly remarkable simplicity of the above stored energy function! Second, the resulting theory is f r a m e - i n d i f f e r e n t in the sense that the value of the above stored energy function is unaltered if r := 0 + ~ia' is replaced by Q~,, where Q is any orthogonal matrix of order three (Ex. 9.5). Third, the resulting theory is a large d i s p l a c e m e n t , or equivalently a large d e f o r m a t i o n , t h e o r y in the sense that the de-scaling produces a displacement field that is O(1) with respect to e, at least in a formal sense. Finally, a noteworthy characteristic of the equations found in Thm. 9.4-1 is that their formal linearization produces the equations of the linear "membrane" theory (Chaps. 4 and 5). This is perhaps best seen from the expression of the energy, in which the covariant components Ga~(~/) - 89 aa~) of the change of metric tensor become by definition the covariant components 7a~3(~/) of the linearized change of metric tensor (Thm. 4.5-2). An inspection of the partial differential equations in the associated boundary value problem (Thm. 9.4-2) likewise shows that they reduce to those of the linear theory when 70 = "Yand the middle surface S is elliptic (Thm. 4.5-2).

Remarks. (1) Otherwise the function spaces and the boundary conditions have to be appropriately modified in the linearization process, so that the two-dimensional equations of the linear membrane theory become well-posed over the resulting spaces VM(W) or V~M(W) (Thms. 4.5-1 and 5.7-1). (2) As observed by Miara [1998], another unexpected link with the linearized equations occur if higher-order forces are considered; cf. Ex. 9.6. II Note that Collard & Miara [1999] have shown that the formal analysis of Miara [1998] described supra also leads to the explicit computation of the limit stresses in a nonlinearly elastic membrane shell. The existence theory for the minimization problem is challenging: The energy j ~ is coercive on the space WM(W) (Ex. 9.4), but, as shown by Genevey [1997], j ~ is not sequentially weakly lower semicontinuous on WM(W) (essential to her proof is the non-polyconvexity of the stored energy function of a St Venant-Kirchhoff material es-

Sect. 9.5b]

The two-dimensional equations derived by F-convergence theory 453

tablished by Raoult [1986]). Hence the fundamental theorem of the calculus of variations cannot be applied (by contrast, this theorem can be successfully applied to nonlinearly elastic "flexural" shells; cf. Sect. 10.6). Another tool that is sometimes successful for proving existence theorems in nonlinear elasticity is the implicit ]unction theorem applied to the associated system of partial differential equations~ which in the present case is quasilinear (Thm. 9.4-2). But, even though the existence and regularity results for the linearized equations of a linearly elastic elliptic membrane shell are firmly established (Thm. 4.5-1), the implicit function theorem cannot be applied to the nonlinear membrane shell equations, expressed as a set of three nonlinear partial differential equations together with the boundary conditions ~ - 0 on 7, if only because the boundary condition ~ - 0 on -), is "lost" in the linearization. As a result~ the derivative at ~e _ 0 of the associated nonlinear operator is not an isomorphism between the "right" spaces, i.e., those of the linearized boundary value problem; cf. Genevey [1997]. As shown by Coutand [1997b, 1999b, 1999c, 1999d, 1999e] in the planar case~ the implicit function theorem can nevertheless be successfully used in particular situations, e.g., if the forces are themselves planar, or if the boundary conditions ~i = 0 on 9' are replaced by boundary conditions of "planar tension". Again in the planar case when ~ is a disk and V0 = ")'~ Genevey [1998] has likewise shown that the implicit function theorem provides the existence of radial solutions around an explicitly computable nonzero radial solution. Nonlinearly elastic membrane shells may thus be likewise amenable to this approach if the applied forces, or the boundary conditions, or the middle surface, are of special kinds.

9.5 ~.

THE TWO-DIMENSIONAL EQUATIONS OF A NONLINEAttLY ELASTIC MEMBRANE SHELL DERIVED BY MEANS OF r-CONVERGENCE THEORY~ COMMENTARY

A remarkable progress in the asymptotic analysis of nonlinearly elastic shells is due to Le Dret & Raoult [1996], who gave the first proof of convergence as the thickness approaches zero. In so doing, they extended to shells the analysis that they had successfully ap-

454

Nonlinearly elastic membrane shells

[Ch. 9

plied to "nonlinearly elastic planar membranes" in Le Dret & Raoult [1995a] (see also Vol. II, Sect. 4.13), where they had likewise given the first convergence result in the planar case. Note that their analysis has since then been extended by Ben Belgacem [1997! and E1 Bachari [1997, 1998] to stored energy functions such that W ( F ) -+ +cr as det F --~ 0 + and to junctions between shells and multi-layered shells. More specifically, H. Le Dret and A. Raoult showed that a subsequence of deformations that minimize (or rather "almost minimize" in a sense explained below) the scaled three-dimensional energies weakly converges in W I , P ( ~ ) as e -+ 0 (the number p E]I, cr is governed by the growth properties of the stored energy function). They showed in addition that the weak limit minimizes a "membrane" energy that is the r-limit of the scaled energies. We now give an abridged account of their analysis. Let w be a domain in I~ 2 with boundary 3' and let 0 E C2(~; I~3) be an injective mapping such that the two vectors an(y) = OaS(y) are linearly independent at all points y = (Ya) C ~. For each ~ > 0, we define the set :=

,,,x] -

e[,

we let z e -- (m~) denote a generic point in the set ~e and we let O~ "= O/Oz~; hence z ae - y a and 0~ - On. Consider as in Sect. 8.3 a family of elastic shells with the same middle surface S = 0(~) and whose thickness 2e > 0 approaches zero. The reference configuration of each shell is thus the image O ( ~ ~) C R 3 of the set ~e C li~3 through a mapping O 9~e -+ IR3 defined by O(x e) : : 8(y) + x~a3(y) for all x e - (y, x~) - (yl, y2, x~) e ~e. By Thm. 3.1-1, if the injective mapping 8 9~ -+ ~3 is smooth enough~ the mapping 0 9 -+ ~3 is also injective ]or e > 0 small enough and yl, y2, m~ then constitute the "natural" curvilinear coordinates for describing each reference configuration O ( ~ e). Assume that the shells are made for all ~ > 0 of the same hyperelastic homogeneous material, satisfying the following properties (hyperelastic materials are studied in detail in Vol. I, Chap. 4): Let 1~ 3 denote the space of all real square matrices of order three and let J. I denote any norm on 1~3; it is then assumed that the stored energy ]unction l~ 91~ 3 --+ I~ of the hyperelastic material satisfies the

Sect. 9.5 b]

The two.dimensional equations derived by P-convergence theory 455

following assumptions: There exist constants C > 0, a > 0, ~ E I~, and 1 < p < cx~ such that [W(F)[ ~ C(1 + [F[p) W(F) ~ ~IF[ p + / 3

for all F E 1~3, for a l l F E l ~ 3,

l~r(F) - ~7(G)[ ~ C ( I -~-IF[ p-1 + [G]p-1)[F - G[

for all F, G E M 3. It can be verified that the stored energy function of a St VenantKirchhoff material, which is given by I~(F)-

A {tr (FTF - I) }2 ~p tr ( F T F - I) 2 -{--~

satisfies such inequalities with p - 4; cf. Ex. 9.7. By contrast, the stored energy function of a linearly elastic material, which is given by

W ( F ) - P IIF + FT - 2III 2 + gA {tr (F T + F -

211} 2

where ]IF]] "- {tr F T F } 1/2, satisfiesthe first inequality with p - 2, but not the second one. It is further assumed that, for each s > 0, the shells are subjected in their interior to applied body forces of density ~ : (/~)" ~ -+ R 3 per unit volume, where f~ E Lq(~ e) and ~1 + ~1 : 1. Since these densities do not depend on the unknown, the applied forces are dead loads (Vol. I, Sect. 2.7). Applied surface forces on the "upper" and "lower" faces of the shells could be likewise considered, but are omitted for simplicity; see in this respect Le Dret & Raoult [1996] who consider a pressure load (cf. Appendix in ibid.), an example of applied surface force that is a live load (Vol. I, Sect. 2.7). Finally, it is assumed that each shell is subjected to a boundary condition of place along its entire lateral face 0 ( 7 • [-~, s]), i.e., that the displacement vanishes there. For each ~ > 0, let :=

let ~ - (~) denote a generic point in the reference configuration { ~ } - , let 0~ "- 0/05~, and let the deformation gradient associated with any deformation ~b~ - ( r { ~ } - --+ ]~3 of the reference

456

[Ch. 9

Nonlinearly elastic membrane shells

configuration be the matrix field ~e~be" { ~ } - -+ 1VIIs defined by ^~ ^~ 01~1 ^,^, 01~2 ^ ^

"--

^~ ^e 02~1 ^,^, 02 ~2 ^e ^e

o2r

03~b "e "e1 0^'3 ~^ 2' ^ ^

9

The three-dimensional problem is then posed as a minimization problem in terms of the unknown deformation field

~" "= i d ~ + ~

of the reference configuration, where ~e . {~e }- __+ IR3 is its displacement field: It consists in finding ~be such that

~

E ~(~e) and .~e(~e) _

0 is said to r - c o n v e r g e as e --+ 0 if there exists a functional J : V --+ i~ U {+c~}, called the r - l i m i t of the functionals J(c), such that ,(e) -+ -+ 0 j(,) < ~--+0

on the one hand and, given any v E V, there exist v(e) E V, ~ > 0, such that vie/.. --+ v as e --+ 0 a n d Jlvl.. = lim J/e~/v/e//,...... s--+0

on the other. As a preparation to the application of r-convergence theory, the scaled energies J ( s ) " ~7V(12) --+ I~ are first extended to the larger space L p (~2) by letting J(e)(O)

-

{

J(e)(O) if ~ e W(~2), +c~ if ~ e IF(l]) but ~ ~ W(~2).

Such an extension, customary in r-convergence theory, has inter alia the advantage of "incorporating" the boundary condition into the extended functional. Le Dret & Raoult [1996] then establish that the family (J(e))e>0 of extended energies r-converges as ~ -~ 0 in LP ( ~ ) and that its r-limit can be computed by means of quasiconvex envelopes. More precisely, their analysis leads to the following remarkable convergence theorem, where the limit minimization problems are directly posed as two-dimensional problems (part c)); this is licit since

Sect. 9.5 b]

The two-dimensional equations derived by F-convergence theory 461

the solutions of these limit problems do not depend on the transverse variable (part (b)). Note that, while minimizers of J(e) over ~r(f~) need not exist, the existence of a "diagonal infimizing family" in the sense understood below is always guaranteed because infvc~r(n ) J ( e ) ( v ) > - o o . In what follows, the notation (bl; b2) stands for the matrix in 1V[[3• with bl, b2 (in this order) as its column vectors and v/-ddy denotes as usual the area element along the surface S. T h e o r e m 9.5-1. Assume that there exist C > 0, c~ > 0,/3 E ~, and 1 < p < c~ such that the stored energy function l~ " 1V~3 -+ I~ satisfies the following growth conditions:

IW(F)I ~

C(1 + IF]p)

12V(F) ~ alF[P +/3

IlrC(F)- ff(G)l _< C(1

+

for all F e M 3, for all F C M 3,

IFIp-1 + IGIP-X)IF - GI for all F, G E M 3.

Let the space W(f~) be defined by

W(f~) :-- {~ e Wl'P(f~); ~ -- 0 on -y • [-1, 1]}, and let (s be a "diagonal infimizing family" of the scaled energies, i.e., a family that satisfies

~(~) E ~7~r(f~) and J(6)(~(e))
O,

where h is any positive function that satisfies h(e) --~ 0 as e --~ O. Then: (a) The family (~(e))e>0 lies in a weakly compact subset of the space wl'p(f~).

(b) limit c W(n) sequence of (u(e))e>0 satisfies 0 3 ~ of the transverse variable.

0

e kly o ,e ge t

0 in f~ and is thus independent

462

[Ch. 9

Nonlinearly elastic membrane shells

(c) The vector field ~ "- 89ft_l ~da~3 satisfies the ]ollowing minimization problem (QI~tr0(y, .) denotes for each y E ~ the quasiconvex envelope of 15ro(y,-))" E W~'P(w) and 3M(~)=

~ ( 0 ) - 2 f Qr

inf

0ew~"(~)

3M(rl), where

(a~ + 010; ~2 + 020))Cddy

r

I~0(y, (bl; b2)):= inf lPtr((bt; b2; b3)G-t(9)) bsE~ s

for all (y, (bl; b2)) C w

X

~/~[3•

G ( y ) = ( a l ( y ) , a2(y), a3(y)) ,

the vectors ai(y) forming for each y E -~ the covariant basis at the point O(y) E S. I

It remains to de-scale the vector field ~. In view of the scalings performed on the deformations, we are naturally led to defining for each ~ > 0 the limit displacement field ~e 9_w --+ i~3 of the middle surface S by

It is then immediately verified that ~ satisfies the minimization problem (the notations are those of Thm. 9.5-1): ~e E W ~ ' P ( w ) a n d ' j ~ ( ~ e ) _

inf

0ew]"(~)

3~(0), where

~ ( 0 ) - 2~ [ QWo(y, ( ~ + 0~; ~2 + 02O))~dv r

{

A word of caution. As their three-dimensional counterparts fi(e) and ~, the notations ~e and 0 emphasize that, even though the limit minimization problem is expressed in terms of curvilinear

Sect. 9.5 b]

The two-dimensional equations derived by F-convergence theory 463

coordinates (the coordinates Yo of the points y E ~), the unknowns are no longer the covariant components of the limit displacement field. Instead, the unknowns are now the Cartesian components, i.e., over a fixed Cartesian frame, of the displacement field ~ 9--->w R3 of the middle surface. Likewise, ~ 9f~ -+ I~3 denotes the vector field formed by the Cartesian components of the applied body force density, m A natural question immediately arises: How does this de-scaled minimization problem compare with the de-scaled minimization problem derived in Sect. 9.4 by means of the method of formal asymptotic expansions? As we now explain, it presents similarities with, as well as differences from, the nonlinear membrane theory previously found by formal means. First, it shares with the nonlinear membrane theory of Sect. 9.4 the property that the unknown F/appears only by means of its firstorder partial derivatives Oa~7 in the stored energy function

found in the integrand of the e n e r g y j ~ . It is likewise a large displacement, or equivalently a large deformation, theory in the sense that the de-scaling produces a displacement field that is

0 (1) with respect to ~. Second, assume that the original stored energy function is frameindifferent in the sense that

r162 (RF)

- r162

R e

F e M

where 0 3+ denotes the set of all real orthogonal matrices t t of order three satisfying det t t = 1. This relation is stronger than the usual one, which holds only for F E 1~3 with d e t F > 0 (Vol. I, Thm. 4.2-1); it is, however, verified by the kinds of stored energy functions to which the present analysis applies, e.g., that of a St VenantKirchhoff material. Under this stronger assumption, Le Dret & Raoult [1996, Thm. 10] establish the crucial properties that the stored

energy function found in j ~ , once ezpressed as a function of the points of S, is frame-indifferent and that it depends only on the metric of the deformed middle sur]ace. Hence this theory is also a f r a m e i n d i f f e r e n t , n o n l i n e a r ~ m e m b r a n e " shell t h e o r y , like the one derived in Sect. 9.4 by means of a formal method.

464

Nonlinearly elastic membrane shells

[Ch. 9

It is remarkable that the stored energy function found in j ~ can be explicitly computed when the original three-dimensional stored energy function is that of a St Venant-Kirchhoff material; see Le Dret ~z Raoult [1996, Sect. 6]. It is no less remarkable that Genevey [1997, Thm. 2.2.1] has been able to show that, for such a material, this stored energy ]unction coincides with that found by Miara [1998] (Tam. 9.4-1), provided that the singular values of the limit deformation gradients belong to an ad hoc compact subset of I~2, which can be explicitly identified (Le Dret & Raoult [1995a, Prop. 16] had already made a similar observation in the planar case). As a result, the linearization of the present nonlinear membrane theory does not always produce the equations of the linear "membrane" theory, by contrast with the nonlinear membrane theory of Sect. 9.4 (see the commentary at the end of ibid.). A w o r d of c a u t i o n . These two approaches thus provide an intriguing instance where the limit equations found by a formal asymptotic analysis do not always coincide with those found by a convergence theorem. This is all the more puzzling, since the original threedimensional equations, the scalings, and the assumptions on the data are the same! m Le Dret & Raoult [1996, Sect. 6] have further shown that, if the stored energy function is frame-indifferent and satisfies I~(F) ~ l~(I) for all F E 1~3 (as does the stored energy function of a St VenantKirchhoff material), then the corresponding shell energy is constant under compression. This result has the striking consequence that "nonlinear membrane shells offer no resistance to crumpling. This is an empirical fact, witnessed by anyone who ever played with a deflated balloon" (to quote H. Le Dret and A. Raoult). This is why the equations found by Le Dret & Raoult [1996] seem to be especially appropriate for membrane shells made with a "soft" elastic material, but this assertion is yet to be rigorously established. Indeed, the modeling and numerical simulation of shells made of "soft", or "rubberlike", elastic materials is of paramount importance as they are so often encountered in practice; think of, e.g., a trampoline, a sail, or a tire! In this direction, see Muffin [1991], Schieck, Pietraszkiewicz ~ Stumpf [1992], Basar & Itskov [1998], Antman & Schuricht [1999].

465

Ezercise8

Another challenging open problem consists in determining whether I~-convergence theory could produce a two-dimensional "flexural" theory of nonlinearly elastic shells~ analogous to the theory (described in the next chapter) obtained through the formal approach.

EXERCISES

9.1. Let J~ - ( f a ) e C2([0, 1]; R 2) be an injective mapping such that f ' ( t ) ~ 0 for all t e [0, 1] and let S - 0(~), where w =]0, 1[• 1[ and 8(t, z) - f a ( t ) e a -F z e 3 for (t, z) e ~. The surface S is thus a portion of a cylinder orthogonal to~ and passing through, the planar curve f([0, 1]). Finally, let 70 C 7 be such that {(~, 0) ~ R2; 0 _< t _< 1} u {(~, 1) ~ R~; 0 ___ ~ _< 1} c ~0. Show that the manifold { ~ - ( ~ ) e I ~ ( ~ ) ; ~ - o on ~0, ~ , ( ~ )

- ~,

- 0 i~ ~ ) ,

which contains the manifold ~40(w) (Sect. 9.1), reduces to {0}. This exercise (due to D. Coutand) thus provides an instance of a nonlinearly elastic m e m b r a n e shell (Fig. 9.1-1). 9.2. Let w be a domain in R 2, let V0 be a subset of ~, - Ow, and let 0(yl, y2) - (yl, y2, 0) for all (yl, Y2) E ~. Show that the manifold {W - (r/i) E Hi(w); ~ - 0 on ~0, aa[3(~) - ~a[3 - 0 in w} reduces to ~0} if V0 = ~ or if V0 C ~ has the following property: There exists (at least) one direction such that the intersection of with any line parallel to this direction is a (finite, since w is a domain) union of segments whose end-points belong to 70. This exercise (due to C. Mardare) shows that a plate subjected to a boundary condition of place along a "sufficiently large" (in the above sense) portion of its lateral face constitutes an instance of a nonlinearly elastic membrane shell (Fig. 9.1-2). 9.3. The notations used in this exercise should be self-explanatory. Let a surface S - 0(~) - 0({5~}-) be equipped with two systems of

Nonlinearly elastic membrane shells

466

[Ch. 9

curvilinear coordinates (ya) e ~ and (Ya) e {~}- and assume that

O(yo) 0(~0). -

Show that 0~0(~o) = {0} implies that .A40(~) = {0} (the manifold .h,'t0(w) is defined in Sect. 9.1). This means that the definition of a nonlinearly elastic membrane shell (Sect. 9.1) is independent of the system of eurvilinear coordinates employed for representing the surface S.

9.4. The scaled two-dimensional energy jM of a nonlinearly elastic membrane shell is defined by (the notations are those of Thm.

9.3-1): 1 ~ aa~ r jM(rl) -- g (aar(rl) -- aar)(aa~(rl) -- aa~)~rddy

- ~ Pi'~ Show that there exist constants a > 0 and fl E IR such that _

, ~(~) + 3

for aU ~ e WM(W) -- {~ -- (~i) e Wl'4(w); ~ -- 0 on 70}. Remark. The energy jM is thus coercive on the space WM(W). Genevey [1997, Thin. 1.4.3] has shown that it is not weakly lower semi-continuous on WM(W), however (analogous properties hold in the three-dimensional case; cf. Ex. 8.1). 9.5. Show that the stored energy function of a nonlinearly elastic membrane shell, viz.,

-(~i) e wl.4(~) -+ ~ ~ ' ~ . ~ ( ~ ( ~ ) - ~ . ~ ) ( ~ ( ~ ) - ~,). is ]tame-indifferent, in the following sense: Given any ~ E w t ' 4 ( w ) , its value is unaltered if r := O + yia s is replaced by Q r where Q is any orthogonal matrix of order three. 9.6. This exercise shows that, if higher order forces are considered, the leading term of the formal expansion of the scaled unknown (then also of a higher order) satisfies the equations of a linearly elastic "membrane" shell found in the linear theory (Thm. 3.4-2). This observation is due to Miara [1998, p. 352].

467

Ezercises

Let the assumptions be as in Thm. 9.2-1, save that the applied body and surface force densities are now such that 9

/"e(x~) -- s r f " r ( x ) for all x ~ - 7r~x E ~ e hi'~(x e) = g l + r h i ' l + r ( x ) for all x ~ - 7rex E F~_ U F e

where r is an arbitrary integer ~ 1 and the functions fi, r E L2(~) and h i'l+r E L2(F+ U r _ ) are independent of s. (1) Show that the leading term of the formal asymptotic expansion of the scaled unknown u(s) is u r (in particular then, u ~ vanishes). (2) Show that u r 9 ~ ~ I~3 is independent of the transverse variable and that, once identified with a function ~r . ~ _~ ]~3, it satisfies the variational problem:

(~r E W M ( W )

-- {~7 E WI'4(w); W - 0 on 70},

for all ~ - (7/i) E WM(W), where the functions ")'a~(W) are the covariant components of the linearized change of metric tensor associated with a displacement field 7/ia ~ of S and pi, r _

/ f,,r " d~3 + h~ 1+~ +

h i_ , l+r

and h~ 1+~ - h"" 1 + , (., •

1

9.7. Let 1V~3 denote the set of all matrices of order three, let I" [ denote any norm on 1~3, and let the mapping T~r 9M 3 -+ R defined by W ( F ) - ~ P tr ( F T F - I )

2 § ~ {tr (F T F - I ) }

2 fora11FE M3

denote the stored energy function of a St Venant-Kirchhoff material. Show that there exist constants C > O, a > O, and 13 E ]R such that

JIV(F)J _< C(I

+ ]FI4)

II/V(F)I >__ alFI 4 -l-/3

for all F E l~ 3,

for all F E l~ 3,

[I~(F) - lSr(G)l ~_ C(1 + [FI 3 -$-IGI3)IF - GI for all F, G E M 3. Remark. Such a stored energy function thus satisfies all the assumptions needed in Thin. 9.5-1, with p = 4.

This Page Intentionally Left Blank

C H A P T E R 10 NONLINEARLY

ELASTIC

FLEXURAL

SHELLS

INTRODUCTION

The purpose of this chapter is to identify and mathematically justify the two-dimensional equations of a nonlinearly elastic "flexural" shell. To this end, we follow the approach of V. Lods and B. Miara, who showed how these may be obtained through the method of formal asymptotic expansions. Given a surface S - 0(~) and a displacement field rlia i of S with smooth enough covariant components ??i : w ~ I~, let aa#(~?) denote the covariant components of the metric tensor of the associated deformed surface (0 + ~iai)(-~) and let 1

denote those of the associated change of metric tensor. Consider a nonlinearly elastic shell with middle surface S, subjected to a boundary condition of place along a portion of its lateral face with 0(70) as its middle curve, where 70 C 7. Such a shell is a nonlinearly elastic "flezural" shell if the manifold ~F(60)

-- {?7 -- (77i) E W 2 ' 4 ( ~ g ) ;

F/ "-- O v ~ -~ 0 O12 "~/'0,

aa~(r/) - a a ~ = 0 in w}

contains nonzero elements and possesses nonzero tangent vectors at each one of its points (Sect. 10.2). The condition 2~4F(w) # {0} means that there exist nonzero displacement fields rli ai of the middle surface S that are admissible and ineztensional~ i.e., that satisfy ad hoc boundary conditions along the curve 0(70 ) (these boundary conditions are interpreted in Sect. 10.5) and that leave invariant the metric of S. This definition is motivated by a careful analysis (Thins. 10.1-1 and 10.1-2) of the remaining steps needed to complete the induction begun in Chap. 8 when the shell is not a "membrane" one according

470

[Ch. 10

Nonlinearly elastic flezural shells

to the definition given in the previous chapter. More precisely, the formal asymptotic analysis begun in Chap. 8 is concluded as follows when the shell is a "flexurar' one (Thm. 10.3-4): Assume that the manifold .A4F(w) does not reduce to {0} and that it possesses nonzero tangent vectors at each one of its points. Then the contravariant components of the applied body forces must be of the form f i ' e ( X e ) : ~2fi'2(X) for all x e - 7rex C ~ ,

where the functions fi, 2 a r e independent of s (for simplicity, we assume in this introduction that there are no surface forces), the

leading term u ~ 9-~ --+ R 3 of the formal asymptotic expansion of the scaled unknown is independent of the transverse variable, and ~o _- !2 f1-1 u~ dxs satisfies the following (scaled) two-dimensional variational problem of a nonlinearly elastic "flexural" shell: r

C ~4~v(w) - {~ E W2'4(w); U - 0vVl - 0 on Vo, Gaf3(y) - 0 in w},

3

a

Rar((:o) ( ( R b a ~ ) ( r 1 7 6

for all y - (Yi) E Tr V 0, L r designates the linear form defined by

Lr(v) :- f

fi, rviv/-ddX + f r

+ur_

hi, r+lvi~rddr

where it is understood that the functions fi, r and h i'r+t respectively belong to the spaces L2(12) and L2(r+ u r_) and that they are independent of e. Finally, recall that ~?alt/3 - 0/3~?a - F ~ / 3 y ~ - ba/3y3 and Y311/3- 0/3y3 + b~y~. Our point of departure is Thm. 8.8-1, amended as indicated in Thm. 10.1-1. Before continuing the induction proper (part (v)), we take a closer look at the cancellation of the coefficients of -1 and e ~ (parts (i)to (iv)):

478

[Ch. 10

Nonlinearly elastic flezural shells

(i) When Vg.A,'to(w) r .[0} at each r e 2r

the cancellation of

the coefficient of I leads to the following supplementary conclusions: First, Ei~13 = 0 i n f / . Second, the coefficients u roll3 (~ of e ~ in the formal ezpansions of the functions umll~(e) are given by (the functions (i~l~ are ede ned i n ~ / .

•(0)1113 =

-(1 +

aa2 0

0

Ia112)I3111q-

aa2 0

0

iafll~3112'

~(0) aal 0 0 aal 0 0 2113 = - ( 1 + I,~111)I3112+ I,a112~3111, u(o) o a~l o o Third, the term of order one in the formal ezpansion of u(e) is of the form u1= r

r

= (r r

z3r

_

with r E W(w) and r

E W(w),

i, given t,y a

0

a

0

:= bl(a

_a2J-O ~ 0 _ a a 2 + (1 + a qa112)~3111

_alJ.O

r 0 :-- b2 Ca + (1 + a r _ aala~2 r := _ o r

0 0

_ aal

-

0

0

0

0

0

0

~c,111~3112, ~all2i3111,

Finally, ~0 E .A,"I.F(w) := {r/E W2'4(w); r / - Our/= 0 on 70, Gag~(~/) = 0 in w). To prove that E~I 3 - 0 in ~ simply recall that we showed in part(ii) of the proof of Thin. 8.8-1 and in Thin. 10.1-1 that E~ s - 0 and )~a~E~ ~ + ()~ + 2/~)E~ a - 0 in f~, and that the assumptions 2r C ~/to(W) imply that E~

~ {0} and qFCJ~4o(w) ~ {0) at all

- Ga~(~ ~ = 0 in w, hence in f~.

Sect. 10.1]

A two.dimensional problem satisfied by the leading term

479

The equations 2E~ll3 -- 0 take the form of a nonlinear system with respect to the functions u l ~ , viz., u(o) 0 -4- a ~176 lu (~ 0., (0) II13 -I-- ~'3111 ~I13 --I-- ~'3111=3113 -" O, u(o) o + a ~ o . . u(O) o ~ (o) 2113-4-~3112 all2 /3113 -t-~3112`.3113 - - 0 , (0) aa/3u(O),(o) -4- (o) ( o ) _ O, u3113 -ta113-/311s ual13U3113

where r Ii~ - a~r ~ _ r ~~ r _ bozio i

u(O)

~nd

all3 - 03ua + bai ~ and

i~llZ - a ~

+ b~: ~

(o) = 03u~ "3113 ,

0 3 = ~0illl3' which follow from Osu ~ - 0 in gt have and the relations Uilll been used. As we shall see in part (ii), this nonlinear system can be ezplicitly solved, thanks in particular to the relations E all~ ~ = 0 More (0) satisfies a quadratic equation, specifically, one first shows that "3113 viz.,

(

~(0)~ 2 ( ..al3r0 aala/32 0 0 )2 1 + `.3113] -- 1 + ~ ~alll3 + (~alli~ll2- ~all2 0 and # > 0 and the functions fi,2 E L2(fl) and h i, 3 E L2(r+ Ur_) are again independent of e and t is an arbitrary real number. Besides the analysis that led to Thm. 10.1-2 shows that these assumptions on the data are the only ones possible for nonlinearly elastic flexural shells. 10.3.

THE TWO-DIMENSIONAL VARIATIONAL PROBLEM

EQUATIONS

AS A

It was shown in Thin. 10.1-2 that, when ~t0(w) ~ {0} and ~Fr contains nonzero functions at each ~ E 2~0(w), the leading term of the formal asymptotic expansion of the scaled unknown u(e) is independent of the transverse variable x~ and may thus be identified with a function r of two variables; it was further shown in ibid. that ~0 belongs to the manifold ~ t F ( w ) C M0(w) and that r satisfies ad hoc variational equations for all rl E ~r C ~r The definition of a nonlinearly elastic flexural shell given in the previous section precisely ensures that this variational problem makes sense for such a shell. It remains, however, to shed a brighter light on the somewhat mysterious functions/~0all~ and/~0a[[~(rl) appearing in the variational

Nonlinearly elastic flezural shells

508

[Ch. 10

equations of Thm. 10.1-2: In the same manner that the functions E~ IIf3 and Fallf3(Vl) 0 occurring in the variational equations of a nonlinearly elastic membrane shell are simply equal to G ~ ( r ~ and a ,z~ ( r 0 )rl (Thin. 9.1-1), where G~(,7)

1

- a~)

- ~(a~('7)

are the covariant components of the change of metric tensor associated with a displacement field ~?iai of the middle surface, the functions /~~IIf3 and Fallf3(17) ^0 have definitely more illuminating expressions and interpretations, notably in terms of the covariant components R.,(o)

= bo,(n) - b.,

of the associated change of curvature tensor (see notably Thms. 10.3-1 and 10.4-1). The following result takes care of the functions E~ As stated here, it extends Lods & Miara [1998, Thm. 2], in that I prove that it holds not only for the leading term ~0, but in fact for any element 17 in the manifold 2vtF(w). This extension is particularly convenient for interpreting the two-dimensional equations as a minimization problem (Sect. 10.4). Note that the intricate expressions given in the next theorem for the functions R~f3(17) can be considerably simplified; cf. Thin. 10.3-2. 10.3-1. Let w be a domain in I~2, and let 0 E C3(~; ~3) be an injective mapping such that the two vectors aa - OaO are final Aa2 early independent at all points of-~, let a3 -- la I A a21' and let the Theorem

vectors a i be defined by a i . a j - J~. Given a displacement field ~Tiai of the surface 0(-~) with smooth enough covariant components yi "-~ ~ IR and such that the two vectors aa(rl) := Oa(O + Oia i) are linearly independent at all points of w, let the covariant components of the c h a n g e of c u r v a t u r e t e n s o r associated with this displacement field be defined by : =

-

where bao and ba~ (0) are the covariant components of the curvature tensors of the surfaces 0(-~) and (0 + ~Tiai)(-w) (Fig. 2.3-1).

Sect. 10.3]

The t w o - d i m e n s i o n a l equations as a variational problem

509

Then the vectors aa(~l) are linearly independent, and consequently the functions ba#(~l) and Ra#(~7) are well defined, for all ~1 E .A4F(W). Let the functions R~# (~7) E L2 (w) be d e ~ a ~o~ ~ y o e W ~' ~(~) by 1

{TT

p, 1 +(r:~ ~ + ~1 a m n {r~oo.ll, + r p,. , 1~11o})~,

where ~11~ "= 013r/~ - r-a[3~l~- ba[3~13and ~7311~:- 0[3~73A-b~l~, the functions Fall,(r/, r E L2(w) are defined for any 17 E W2'4(w) and any r E wl'4(og) by

1 "-- ~(r

Fall/3(r/, r

and finally, the field r E W 2 ' 4 ( O g ) by

-f- r

-f- amn{71mllaCnll# + ~Tnll#r (~bi(n)) E wl'4(6g) i8 defined for any

r := b~r/a + (1 + aa2rlall2)rlzllI - aa2r/alll~3ll2, ~/32(Ir/) :'-- b'~rla + (1 + aalr/alll)r/31l 2 - aalr/all2r/3ll 1, r : - -aa~rlall~ - aata~2 (rlalll rl~ll2 - r/all2r/~lll). Then

R~(~)-

R ~ ( ~ ) for a11 ~ E , ~ F ( w ) .

Let the functions ~oall~ E L 2(w) be those appearing in the variational problem satisfied by the leading term ~o E ~4F(w) (el. Thin. 10.1-2; their definitions are given in part (iv) of its proof), viz., /~0

.

0

1 err

0

+(r:b~ + ~1 a m n flap, , ' ~ -1/'0 ,,,

0

+ r~

o

510

[Ch. 10

Nonlinearly elastic flezural shells

where 1

F~ r

_mnr~O

:= ~(r/alll3 + r/~l[a -f- a := (r with r ._ r

0"

(~m[[a~ln[[[3+ ~nli/3~lm[la}),

Then

~~ ~ - R~,(r o) = R~,(r176

^o ~ - Ra~(~ b Proof. That E,~II ~ immediately follows from the defi-

nitions of the functions R~13(~/) and/~0

It thus remains to show

that ba13(r/) is well defined and that R~(~/) - ba~3(~/)- bal3 for all n ~ A4F(~). (i) For any '1 E A 4 y ( w ) , the vectors aa(~l) are linearly independent at all points in-~. Since the set ~ is compact, the assumption that the vectors aa E C2 (~; I~3) are linearly independent implies that there exist constants Cl and c2 such that 0 0 in where ha(y) "- Oa(e + ~?ia'). These relations imply in particular that

= b.,(n)

-

= R.,(,)

.

e

as was already established in Thm. 10.3-1. Proof. The proof follows the same lines as that of Thm. 10.3-1. If, instead of the relations haft(y) -aaf3 = 0 in w, a vector field rl E W 2' 4(w) satisfies the less restrictive relation

a(rl) := det(aafj(Vl) ) > 0 in w, then the vector a3(~) and the functions ba~(~7) are now given by (compare with parts (ii) and (iii) of the proof of Thm. 10.3-1, whose notations are employed here): i a3(~7)-

aa(~7)Xi(~)ai,

516

[Ch. 10

Nonlinearly elastic flezural shells

so that (compare with part (v) of the proof in ibid.) a

II

for such a vector field, and the assertion is established.

The next result, due to Lods ~ Miaxa [1998, Thin. 3], takes care of the functions F_ ~^0 iif~(~7). ..

Let the functions R ~ ( y ) e L 2 ( w ) b e def i ~ e d f07" a ~ y ~7 ~ W2'4(~g) as i~, Thin. 10.3-1 and let the functions ~o11~(,~) ~ L~(~) b~ tho,~ a ~ ~ i , ~ i,~ th~ ~a~atio,~t ~q~atio,~, ~tisfied for all ~1 ~ T~0c~e(w) by the leading term ~o ~ .~te(w) (cf. Thin. 10.1-2; their definitions are given in part (vi) of its proof), viz., Theorem

10.3-3.

1

(p,1

I am n y~p, 1/,0

I am n

0

O'7"

~ pp, 1 0

FP, 1 [,O

~q, 1 0

where F2I

l

i~('~) "= ~(~ii, + ,7~11~+

a mn

0

{i.,il~'7.1i~ + r

r/ailf3 :-- OfP7a -- r aaf3~70- - ba/3~73,

~73iif3:-- 0f3~73 ~- b~r/0-

and the fields ~0(~/) _ (~o(17)) e W(w) and r given by:

v0(,)

0

e W(w) are

= (r

.= b?,o + ,~ll~ +~"~(r

+ i~

- i3~

~ - i~

+aal (~~

-I- (:~

- (:~ lvlail2 - ~all2~Taill),

o

~~ (~7) :---aaf3~Tallf3 -aala~2(~'a~

2 + ~'f~li2~Talll- ~~

- ~f~lll~Tal12),

Sect. 10.3]

The two-dimensional equations as a variational problem

r

:= r (~o) _ b~.o + (1

+ aa2(~~176

r

: : r162

+ aal(~Ojll)(~30]]2

= b~r + (1

r 0 :--- r

----aCZ/~iOi]/~

aal -

-

517

1 -a-a2 v.o~aj]l~-3]02,0 -

aalr

-

0 0 0 0 a/~2(~aJ]l~/~ll2 ~ai]2~/~]}l)" -

-

Then

#~

-

(R~) , (~0)y for all y e Vr ~

where (R~f~)'(~"~ designates the Frdchet derivative at r of each mapping R~/~ " W2'4(w) -+ L2(w).

e .h4v(w)

Pro@ For details about the notions of differential calculus used in~a, see, e.g., Vol. I, Sect. 1.2. The functions R~af3(v$) are of the form

R~(,~) - a~,,~(,~)+ H~,,~(~), where

a~it~(n ) .- F.it~(., r 1

ar

i

+ ( r ~ ~+ ~

a m n.f~p, 1

p, 1

~-~o,-11~+ r.~ ,~t,o}),~.

The mappings (~7, ~ ) " W2'4(w) • wl'4(w) -+ Fall/3(~, ~) E L2(w) are affine with respect to 17, linear with respect to ~, and continuous; hence they are differentiable. As a sum of continuous linear and quadratic mappings, the mapping ~ 9W2,4(w) -+ w l , 4 ( w ) is likewise differentiable. The expressions of the G gteau.x derivatives for such functions together with the chain rule then give

a'lt~(r fo~ an r

-

Fo,t~(r r162

~ w2,4(~). Be~ide~ (Thin. 10.V3), r162

C W2'4(0~),

_ ~o0(.) for a l l . E ~r

so that

r~ll~(r ~ r162176 for a11 ~ E qF~o~F(w).

FoiI~(r 0, ~,~

-

Foll~(v,o(,7))

518

[Oh. 10

N o n l i n e a r l y elastic f l e z u r a l shells

As sums of continuous linear and quadratic mappings~ the mappings Hall3 " W2'4(w) --+ L2(w) are differentiable and their G~teaux derivatives are given for any ~, ~/E W2'4(w) by 1 (rr

lamn

+ (r:~~ + ~

p, 1

{r~or

1 _mn r~p, 1

+ r~.~~r

l~p, 1

Combining the above relations thus yields

R~e(r

_ a.lle(r

+ H. le(r

_ p0

for all rl E T~;o.h4F(w) and the proof is complete.

I

We are now in a position to recast the variational problem of Thm. 10.1-2 in a more suitable form, as an immediate corollary to Thms. 10.3-1 and 10.3-3: T h e o r e m 10.8-4. Consider a family of nonlinearly elastic flezural shells according to the definition of Sect. 10.2, with thickness 2~ > O, with each having the same middle surface S = O(~) and with each satisfying a boundary condition of place along a portion of its lateral face having the same set {?(To) as its middle curve, and let the assumptions on the data be as in Sect. 10.2. Finally, assume that 0 ~ Ca (~; I~3). Then the leading term u ~ of the formal asymptotic ezpansion of the scaled unknown u(e) is independent of the transverse variable x a and ~o "-._ !2 f l 1 uO dx3 satisfies the following sealed twod i m e n s i o n a l v a r i a t i o n a l p r o b l e m T'F(w) of a n o n l i n e a r l y elastic flexural shell: ~0 C .M.F(W)"-- {~ C W2'4(W); ~ -- ~ , ~ -- 0 on "Yo,

o , ~ ( n ) = o i~

1L

a3~r b

L

'

"

for all r / - (r/i) E T r Vr

:= {n c w~,4(~o); n

~},

where

- o ~ n = o oll "to,

G'/3(r176

0 in w},

Sect. 10.4]

The two.dimensional equations as a m i n i m i z a t i o n problem

519

1 where the functions Oa~ (0) -- ~ (aa# (~1) - aa#) and R~a#(~1) are defined in Thins. 9.1-1 and 10.3-1, and finally, aaf3~rr := ~ 4Xl.t + 2p a~a~rr + 2p(aa~ra~r + aara~r), 9 := pZ,2

i , 3 -4- h i_,3 a n d h ~ 3 " - h z'"3 (., -4-1). f z ,92 d x 3 + h.,%

1

E

10.4.

T H E T W O - D I M E N S I O N A L E Q U A T I O N S AS A MINIMIZATION PROBLEM

A crucial property has yet to be exploited: When a field ~1 = (~}i) belongs to the manifold .h4F(w), the functions R~f3(17) become equal to the covariant components of the change of curvature tensor associated with the displacement field 7}iai of the middle surface S (Thm. 10.3-1). This goal is achieved in two stages: First, by recognizing as in Lods & Miara [1998, Thm. 3] that the variational equations of problem 7~F(w) (Thm. 10.3-4) express that the Gdteaux derivatives (j~F)'(~~ of an ad hoc functional J~F vanish for all the fields ~7 in the tangent space to the manifold .A/tf(w) at ~0; second, by noting that, over this manifold, J~F becomes equal to a functional jF whose integrand is (apart from its linear terms accounting for the applied forces) a quadratic and positive definite expression, via the scaled twodimensional elasticity tensor of the shell, in terms of the change of curvature tensor introduced in Thm. 10.3-1. These decisive observations in turn allow to recast the two-dimensional variational problem :PF(w) as a minimization problem, which now exhibits a remarkable simplicity. In this minimization problem, which will be studied for its own sake in Sect. 10.6, lies the apex of the application of the method formal asymptotic expansions to nonlinearly elastic flexural shells. T h e o r e m 10.4-1. Given a nonlinearly elastic flezural shell according to the definition given in Sect. 10.2, let the manifold ~&4F(w)

520

[Ch. 10

Nonlinearly elastic flezural shells

and the functional j~ " W2,4(w) --~ I~ be defined by ~v(~)

"- { n = ( ~ ) e w 2 , 4 ( ~ ) ;

n - o~

- o on ~0,

a.z(n) -~,

j~(17) "-- ~

a

R~r(~7)R~f3(.)v/ady-

= 0 i=

~),

p"27Ii~dy

for all O ~ W~,4(w),

where the functions aaf3(17) and Rba[3(n) are defined in Thins. 9.1-1 and 10.3-1 and the functions a a/3ar and pi,2 are defined in Thm. 10.3-3. Then the functional j~ is differentiable over the space W2'4(w) and ~o C .&4F(w) is a solution to the variational problem PF(w) of Thin. 10.3-4 if and only if it is a stationary point of the functional j~ over the manifold ,A,4F(w), i.e., it satisfies (j~),(~o)~/ _ 0 for all in the tangent space ~go,A,4F(w) to the manifold ,h/tF(w) at ~o. Since the fianctions bar3(U) are well defined for all ~ G .A/tF (w) and R~,(n)

= b.~(u)-

b.~ Io~ an ,7 e ~ v ( ~ ) (Tam. 10.3-2), w~tic~t~

solutions to problem 7OF(w) are obtained by solving the minimization problem: Find ~ such that

E ~It~(w) and j F ( ~ ) =

inf iF(v/), where neAav(~)

1 f~ aaf3~r - ~pi,2~Tivfady.

Proof. The differentiability of the functional j~ over the space W2,4(w) is a simple consequence of the definition of the functions R~(v/) (Thm. 10.3-1). An argument similar to that found in the proof of Thm. 8.2-3 then shows that the G~teaux derivatives (j~)'(~)Vl are given by

(j~)'(~)v/- ~

a

Rar(~)((Rba/3)'(~)Vl)v~dy-

p"2rliv~dy

for all ~, ~/E W2'4(w). Hence an inspection of the variational equations satisfied by ~o E A4F(w) for all vl 6 ~ o ~ t F ( w ) (rhm. 10.3-4)

Sect. 10.5]

The two.dimensional equations derived by a formal analysis

521

immediately reveals that they coincide with the equations (jbF)'(r176 : 0 for an ~ e Vr Conversely, if r E .~vtF(w) is a stationary point of the functional J~F over the manifold 2vtF(w), it also satisfies the variational problem 7>F(w) of Thm. 10.3-4, since the argument that led in Thm. 10.3-3 to the relations _

po

all~(~7) for all ~ C Tr

holds in fact if ~0 is replaced by any ~ in the manifold 2vt~(w) (this observation relies in particular on part (iii) of the proof of Thm. 10.1-3). Particular solutions to problem T'F(w) may thus be obtained by solving the minimization problem: Find r such that C ~'tF(W) and j ~ ( ~ ) -

inf

j~(rl).

Since the functionals j~ and jF coincide over the manifold ~ F ( W ) , this minimization problem may be equivalently defined in terms of the functional iF. I

The functional jF : ,A/tF(W) --+ R is called the scaled two-dim e n s i o n a l e n e r g y of a n o n l i n e a r l y elastic flexural shell. We shall see in Sect. 10.6 that the minimization problem in terms of the functional jp is in fact well-posed over a manifold larger than .A/tF(w), in the definition of which the space H2(w) replaces the space W 2' 4 (w). 10.5.

THE TWO-DIMENSIONAL EQUATIONS OF A NONLINEARLY ELASTIC FLEXURAL SHELL DERIVED

BY MEANS

ASYMPTOTIC

OF A FORMAL

ANALYSIS; COMMENTARY

In order to get physically meaningful formulas, it remains to descale the components ~o of the vector field ~0 that satisfies the scaled two-dimensional problems found in Thms. 10.3-4 and 10.4-1. In view of the scalings ui(~)(x)

- u ~ ( x e) for all x e - ~r~x e ~e

522

[Ch. 10

Nonlinearly elastic flezural shells

made on the covariant components of the displacement field (Sect. 8.4), we are naturally led to defining for each s > 0 the covaria n t c o m p o n e n t s ~ 9W --+ IR of the l i m i t d i s p l a c e m e n t field ~e 9 _w --~ i~3 of the middle surface S of the shell by letting (the vectors a i form the contravariant basis at each point of S)"

Cf ._ r

and ~ := era'.

A w o r d of c a u t i o n . As always, the fields ~ := ( ~ ) and ~ - ~f a i must be carefully distinguished! The former is essentially a convenient mathematical "intermediary", but only the latter has physical significance. II Recall that fi,~ E L2(n e) and h i'e E L2(r~_ u r ~ ) represent the contravariant components of the applied body and surface forces actually acting on the shell and that A* and #* denote the actual Lain6 constants of its constituting material. We then have the following immediate corollary to Thins. 10.3-4 and 10.4-1: T h e o r e m 10.5-1. Let the assumptions and notations be as in Thin. 10.3-4. Then the vector field ~ := ( ~ ) formed by the covariant components of the limit displacement field ~ a i of the middle surface S satisfies the following t w o - d i m e n s i o n a l v a r i a t i o n a l p r o b l e m P~(w) of a n o n l i n e a r l y elastic f l e x u r a l shell:

~s E ,/q~F(69)"-- {~ -- (TIi) E W2'4(w); i t / - Ov~ - 0 on 70,

for all v/E ~Fr

:= {~/E

W2'4(w);

n -

0vn -

0 o n "fo, o in

,,,),

Sect. 10.5]

The two-dimensional equations derived by a formal analysis

523

where a.,(n)

1

.-

-

4)~~#~ a,~a~, - + 2/.t~(aa,, a f~r + a,~,a~,~ ),

aC,f~rr, ~ :=

A~ + 2p ~

pi, S ._

f

'~

9

9

.

.

f"~ dx i + h; ~ + h i'~_ and h~ ~ : : h ''~(., +e),

and the functions R~(17) are defined in Thm. 10.3-1. it is a stationary point over the manifold ,h,4F(w) of the functional j~ defined by e3 ~ aa~ar, eR~r(~l)R~(U)V/_~ dy - ~ pi, e71iv/~dy

~07" all ~ -- (~i) e

W2'4(W).

Particular solutions to problem 7~(w) are thus obtained by solving the minimization problem: Find ~e such that (the functions ba~(~/) are the covariant components of the curvature tensor of the surface (0 + ~Tiai)(-~); cf. Thm. 10.3-1)

~6 E .A4F(w) and j~(~e) _

inf

j~(~/), where

~3 f aa~r' (b~r(~l) - bar)(ba~(~l) - ba~)v/-ady

J~(~l) "- -~ J~

- ~ Pi'~?iv~dY"

m

Any one of these problems satisfied by ~e constitutes one version of the t w o - d i m e n s i o n a l e q u a t i o n s of a n o n l i n e a r l y e l a s t i c f l e x u r a l s h e l l (the specific meaning conveyed by "flexural" is given below). The functions 1 Gaff(r/) - ~(aal3(r/) - aa~) and Raf~(r/) - (baf3(r/) - baf~)

Nonlineavly elastic flezural shells

524

[Ch. 10

are respectively the covariant components of the c h a n g e of m e t r i c t e n s o r and c h a n g e of c u r v a t u r e t e n s o r associated with a displacement field yia i of the middle surface S (Thms. 9.1-1 and 10.3-1) and the functions a a ~ ' e are the contravariant components of the t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of t h e shell. The functional j~ 9.A4F(w) --~ I~ is the t w o - d i m e n s i o n a l energy, and the functional

~3 ~ aa~ar'~(b,r'r(W) _ b,rr)(ba~(rl) _ ba~)v~dy is the two-dimensional strain energy~ of a nonlinearly elastic flexural shell. Finally~ the boundary conditions Y -- O~y -- 0 on 7o express that the shell is strongly c l a m p e d along 7o (the geometric interpretation of these boundary conditions is given infra). A major conclusion is thus that~ without any recourse to any a priori assumption of a geometrical or mechanical nature, the method

of formal asymptotic expansions provides a justification of the twodimensional equations of a nonlinearly elastic flexural shell, in the

forms found in Thm. 10.5-1. This justification by Lods & Miara [1998] constitutes a generalization to shells of the formal analysis of Fox, Raoult & Simo [1993] in the planar case, i.e., when the mapping 0 is of the form 0(yl, Y2) = (Yl, Y2, 0) for all y -- (Yl, Y2) E w (see also Vol. II, Sect. 4.12). Further important conclusions and comments are in order about the present justification: First and foremost, the resulting shell theory is a n o n l i n e a r flexu r a l t h e o r y in the sense that the s t o r e d e n e r g y f u n c t i o n of a n o n l i n e a r l y elastic f l e x u r a l shell, defined by:

,-

e

-

-

b.,)

is a quadratic and positive definite expression (via the two-dimensional elasticity tensor of the shell) in terms of the change of curvature tensor, i.e., of the exact difference between the curvature tensor of the deformed middle surface and that of the unde]ormed one, while the associated energy is to be minimized over displacement fields for which the change of metric tensor, i.e., the exact difference between

Sect. 10.5]

The two-dimensional equations derived by a formal analysis

525

the metric tensor of the deformed middle surface and that of the undeformed one, vanishes. The existence theory for this minimization problem is treated in the next section, where further relevant comments are also to be found. Note in passing the truly remarkable simplicity of this minimization problem! Second, the resulting theory is f r a m e - i n d i f f e r e n t in the sense that the value of the above stored energy function is unaltered if, given any r/ = (~7i) E J ~ F ( W ) , ~]~ : = 0 + ~7iai is replaced by Q r where Q is any orthogonal matrix of order three (Ex. 10.5). It is also a l a r g e d i s p l a c e m e n t , or equivalently a l a r g e d e f o r m a t i o n , t h e o r y , in the sense that the de-scaling produces a displacement field that is 0(1) with respect to ~. We now interpret the boundary conditions r/ = 0v r/ = 0 on 3'0. To this end, let rli ai be a displacement field of the middle surface S = 0(~) with smooth enough, but otherwise arbitrary, covariant components TIi : ~ ~ I~. The tangent plane at an arbitrary point O(y) + ~Ti(y)ai(y), y E ~, of the deformed surface (0 + ~Tiai)(-~) is thus spanned by the vectors o

(o +

-

+

+

if these are linearly independent. Since r / = 0v r / = 0 on 3'0 =r ~/i = 0 a r ] i -- 0 on 3'0, it follows that

O(y) + yi(y)ai(y) - O(y) and Oa(O + yiai)(y) - aa(y) for all y e 7o. These relations thus show that not only the points and the tangent spaces (as when only the weaker "boundary conditions of clamping" ~i -- 0u~3 - 0 are imposed on 3'0; cf. Sect. 6.3), but also the tangent vectors to the coordinate lines, of the de]ormed and undeformed middle surfaces coincide along the curve 0('/0). Such t w o - d i m e n s i o n a l b o u n d a r y c o n d i t i o n s of s t r o n g c l a m p i n g are suggested in Figs. 10.2-1 to 10.2.3. The formal linearization of the equations found in Thm. 10.5-1 produces the equations of a linearly elastic flexural shell (Chap. 6). This is perhaps best seen on the minimization problem: In the linearization process, the covariant components Raf3(r/) --- baf3(r/)- bar3

Nonlineavly elastic flezural shells

526

[Ch. 10

of the change of curvature tensor entering the energy become by definition the covariant components paf3(r/) of the linearized change of curvature tensor (Sect. 2.5); likewise, the covariant components Ga~(~l) - 89 - aa~) of the change of metric tensor entering the definition of the manifold J~F(w) become by definition the covariant components 7afj(v/) of the linearized change of metric tensor (Sect. 2.4), so that the energy becomes that of the linear flexural theory (Sect. 6.3) and the manifold .h4F(w) likewise becomes the vector space

vF(

) := { . -

e HI( ) • HI( ) • r/i = 0v7/3 = 0 on 9'0, 7af3(v/) = 0 in w}

of the linear flexural theory (Sect. 6.3)

Remarks. (1) The function spaces and the boundary conditions, which become in the linearization process those of the space VF(W), have to be modified so that the two-dimensional equations of the linear flexural shell theory become well-posed (Thm. 6.3-1). (2) As observed by Lods & Miara [1998], the equations of a linearly elastic flezural shell are also recovered by considering forces of higher order; cf. Ex. 10.6. m Finally, note that Collard & Miara [1999] have shown that the formal analysis of Lods & Miara [1998] described supra also leads to the explicit computation of the limit stresses in a nonlinearly elastic flexural shell. 10.6.

E X I S T E N C E OF S O L U T I O N S T O T H E MINIMIZATION PROBLEM

In this section, which is based on Ciarlet & Coutand [1998], we show that the minimization problem for a nonlinearly elastic flexural shell found in Thm. 10.5-1 has at least one solution, once the manifold ~4F(w) is replaced by a larger manifold, where the space H2(w) replaces the space W2,4(w). For notational convenience, we keep the same notation ,h4F(W) for the enlarged manifold and we suppress in this section all the ezponents "s" appearing in the formulation of this problem. Our point of departure is thus the following:

Sect. 10.6]

Ezistence of solutions to the minimization problem

527

The unknowns are the three covariant components ~i " w -+ of the limit displacement field ~iai of the middle surface S of the shell. This means t h a t ii(y)ai(y) is the displacement of the point O(y) of the middle surface for each y E ~. The unknown vector field :-- (r " w --+ i~3 should then satisfy the following minimization

problem: r ~ A4~(~)

- {,I - (v~) ~ I~2(~); ,7 - o~,i - o o ~ "~o,

aaf~(~/) - aaf3 - 0 in w},

jF(C,)-

inf

n~A4p(w)

jF(rl), where

~3

iF(n)- -~ / aaf3~ (b,;r(rl) - b,Tr)(baf3(rl) - baf3)v/-ddy - L p i r l i ~ dy,

where 70 is a portion of the b o u n d a r y 7 satisfying

length 70 > 0, 0v denotes the outer normal derivative operator along 7, the functions aaf~(~/)" ~ -+ I~ and baf3(Vl)" ~ -+ I~ are the covariant components of the metric and curvature tensors of the deformed surface (O+~liai)(-~) corresponding to an arbitrary field v$ - (v/i) E JV~F(w), aaf }~r :_

4A# aaf3aO.r + 2/z(aa~af3 r + aar a~a ) A+2#

designate the contravariant components of the two-dimensional elasticity tensor of the shell, and finally, the given functions pi E L2(w) account for the applied forces. Two immediate comments are in order about this minimization problem: First, it is clear that the "interesting" situations covered by the present theory are those where the manifold ~/t1~(w) contains other fields ~} than ~} = O. Observe in this respect t h a t such an assumption, which in effect depends only upon the geometry of S a n d u p o n the subset Vo of V, is one of the assumptions made in the definition of a nonlinearly elastic flexural shell (Sect. 10.2).

Nonlinearly elastic flezural shells

528

[Ch. 10

As already noted, this assumption means that there exist nonzero displacement fields 71iai of the middle surface S that are inextensional, in the sense that they preserve the metric of the surface S, and that are also admissible, in the sense that they satisfy the two-dimensional boundary conditions of strong clamping r/ = Our/ = 0 on 7o. This is the case for instance if the middle surface S is either a portion of a cone (excluding its vertex) or a portion of a non-planar cylinder and the shell is subjected to a boundary condition of place along a portion of its lateral face whose middle curve 0(70) is a subset of one of its generatrices (if S is a non-planar cylinder, 0(70) may consist of subsets of two generatrices); cf. Figs. 10.1-1 and 10.1-2 and Exs. 10.1 and 10.2. These developable surfaces constitute canonical examples, but more "exotic" examples can be found; cf. Ex. 10.7. Second, we must verify that the functional jF is well defined on the manifold .A~tF(w). To this end, we will show (part (ii) of the proof of Thin. 10.6-1) that the vectors Oa(O+yia i) are linearly independent if r / - - (7/i) E dg4F(w) and that the functions bat3(r/), which are then well defined, belong to L2(w). It turns out that the existence theory is substantially easier to carry out if, instead of ~ = (~i) and ~1 = (71i), the vector fields

~o "= 0 + ~ia i and '0 := 0 + ~i ai are taken as the new unknown and new "trial functions". In other words, the new unknown is the l i m i t d e f o r m a t i o n field of the middle surface of the shell: This means that ~o(y) - O(y)+ r is the deformation of the point O(y) of the middle surface for each yEW. A w o r d of c a u t i o n . The minimization problem is thus still expressed in terms of curvilinear coordinates (the coordinates ya of the points y E ~), but the unknowns are no longer covariant components (the functions ~i :w --+ I~) over the contravariant bases along the surface S. Instead, the unknowns are now the Cartesian components, i.e., over a fixed Cartesian frame, of the unknown deformation field 3. m Using in particular the relations r/j - (71iai).aj, we remark that the equivalence -

H2(

)

0 +

- r

H2(

)

Sect. 10.6]

Ezistence of solutions to the minimization problem

529

holds, since the assumption 0 E C3(~; I~3) made throughout this chapter (see, e.g., Thm. 10.3-4) implies that ai C C2(~; R 3) and a ~ ~ C2 (~; R ~). If r E H2(w), we define a.e. in w (here and subsequently, the abbreviation "a.e." stands for "almost everywhere") the vector fields

and the functions

~(r

:= . ~ ( r

a,(r

= .~.(r

If r E H2(w) is such that the two vectors a a ( r are linearly independent a.e. in w, we also define a.e. in w the vector field

~(r

~(r "- I~(r

A

~2(r A ~2(r

the functions

and finally, the vector fields ai(r

~(r

by means of the relations

aj(r

i - ~j.

The vectors aa(r and a ~ ( r thus form respectively the covariant and contravariant bases of the tangent plane to the deformed surface r at the point r for almost all y E w.

Remark. I hope, but am not entirely convinced, that I will be forgiven for the lack of consistency observed between, e.g., the notations ai(~7) used so far and ai(r used in this section. At least, these inconsistencies spared me the burden of introducing yet further notations! I We now establish an existence result ]or the minimization problem of a nonlinearly elastic flexural shell, reformulated in terms of the new unknown ~o and trial functions r Note that, for simplicity, we impose only one boundary condition on ~'0, viz., ~o -- ~o0 on 70 (this boundary condition is thus more general than its special case ~o -- 8 on 3'0 considered until now), as the following existence theory holds

530

[Ch. 10

Nonlinearly elastic flezural shells

in this case of a shell that is s i m p l y s u p p o r t e d , as well as in the case (considered so far) of a shell that is strongly clamped. Note also that this existence result holds under a substantially weaker regularity assumption on the mapping 0 than that made so far, viz., 0 6 C3(~; IR3). This assumption was nevertheless essential for carrying out the asymptotic analysis to its term (Thm. 10.3-4). The following ezistence result is due to Ciarlet & Coutand [1998]. It extends to shells the existence theorem established by Coutand [1997a] (see also Vol. II, Thm. 4.12-3) for the minimization problem justified by Fox, Raoult & Simo [1993] in the planar case. The proof is, however, substantially different. The uniqueness or multiplicity of solutions to this problem are studied in Coutand [1999a, 1999f]. T h e o r e m 10.6-1. Let there be given a mapping 0 E W2'p(w; IR3) with p > 2, such that the two vectors a a -- OaO are linearly independent at all points of-~. Let there be given a subset 70 C 7 such that length 70 > 0 and let there be given a mapping 7~o :70 --~ IR3 such that the m a n i f o l d of a d m i s s i b l e i n e x t e n s i o n a l d e f o r m a t i o n s

9

:= {r

e

r

=

on

-

-

0 in

is not empty. Then if r E q~y(W), the vectors a a ( r = 0 a r are linearly independent a.e. in w and the ]unctions ba~ (r are in L2 (w). Given a continuous linear form L on H2(w), define the twod i m e n s i o n a l e n e r g y IF : q~y(w) -~ R of a n o n l i n e a r l y elastic f l e x u r a l shell by

~3 ~ aa~r(b~r(r

- b~r)(ba~(r

- ba~)v~dy - L(r

for all r 6 q~F(w). Then there is at least one 7~ such that

7~ C q~y(w) and I y ( ~ ) =

inf

IF(C).

Sect. 10.6]

Ezistence of solutions to the minimization problem

531

Proof. For the sake of clarity, the proof is broken into a series of seven parts, numbered (i) to (vii). In the first five parts, we establish various properties of the manifold ~F(w), while in the remaining two, we establish properties of the functional IF over this manifold, the combination of which eventually leads to the existence theorem. Note in passing that the properties established in parts (i) to (v) may also be viewed as properties of isometric surfaces. The norms in the spaces L2(w) and Hm(w), rn ~ 1, are denoted as usual I 910,~ and ][. [[m,~ and those in the spaces L~176 and Wl,~176 are denoted I- ]0,oo,~ and I[" I[1,oo,~. The same notations are used for the norms in the corresponding spaces of vector fields, such spaces being then denoted by boldface letters. Strong and weak convergences are denoted by -4 and --~, respectively (a review of all the properties relevant here about weak convergence and lower semicontinuity is found, e.g., in Vol. I, Sects. 7.1 and 7.2). The proof follows a pattern familiar in the calculus of variations: After showing that the manifold ~F(w) is sequentially weakly closed (part (i)), we establish that the functional IF is sequentially

(p ts and (vii)), all these properties holding with respect to the topology of the space H2(w). The existence of a minimizer of Iv over ~F(w) then classically follows from these properties; see, e.g., Dacorogna [1989, Chap. 1] or Struwe [1990, Chap. 1]. Note that the coerciveness of the functional hinges on the crucial property that the manifold 'I'F(W) lies in a bounded subset of W 1, oo(w) (part (iii)).

(i)

of It2( ), the manifold ~F(w) is sequentially

weakly closed, i.e., r

E 'I'F(W), I ~_ 1, and r

___~r in H2(w) =~ r E ~F(w).

Let e l E 'I'F(W), I > 1, be such that e l __~ r in H2(w). Since the trace operator tr from H2(w) into L2(70) is continuous with respect to the strong topologies of both spaces, it remains so with respect to the weak topologies of both spaces (see, e.g., Brezis [1983, Tam. III.9]). Hence tr e l __~ tr r in L2(70) and thus tr r - ~0 on 70 since tr e l _ ~0 on 70 for all I > 1.

Nonlinearly elastic flezural shells

532

[Ch. 10

By the Rellich-Kondra~ov imbedding theorem (see, e.g., Vol. I, Thin. 6.1-5), Ct __, r in Hi(w); hence

~(r

~o(r

-

~(r

-~ ~(r

~(r

- ~o~(r

in Z~(~).

Since a ~ ( r t) - aa~ a.e. in w for all l, we conclude that a ~ ( r - a~ a.e. in w; hence ~ E ~I'y(w) as was to be proved. Should the manifold ,~,(w) include a second boundary condition of the form 0~k : ~01 on 70 (recall that the manifold 2r comprises a boundary condition of the form 0~r/ = 0 on 70), a similar argument shows that such a manifold is again sequentially weakly closed. (ii) There ezists C1 such that, for all vector fields r satisfying aa~ (r - aa/3 a.e. in w,

E H2(w)

0 < c~ ~ la~(~) A a 2 ( ~ ) l ~.e. in ~, C~-~ _< la~(~)l _< C~ a.e. in ~.

Consequently, the vectors ai(~) and ai(~) associated with such vector fields ~ are well defined and "uniformly" linearly independent a.e. in w, the corresponding functions ba~(r are in L2(w), and the functional IF is well defined over the manifold ~ y ( w ) (that the functions ba#(r are indeed well-defined when ~ belongs to the manifold 9 F(w) was already observed in Thin. 10.3-1). Since the set ~ is compact, the vectors aa - OaO are "uniformly" linearly independent in ~ (they belong to the space WI,p(w; R3), which is continuously imbedded into the space Co (~; ~3) since p > 2), in the sense that there exist Cl and c2 such that 0 < cl < 1 and lal 9a21 < ~la~lla21 in ~,

0 < c2 < 1 and c2 < la~l ___c; x in ~. Furthermore, a1(~3),

a2(~3) -

I~x(~)l 2

a12(~3) -

-- a 1 1 ( ~ 3 ) -

la2(~)l 2 --

a22(r

a12 -

all -lal[

al.a

2 a.e. i n w ,

2 a , e , i n w,

-- a22 - - i a 2 l 2 a . e . i n w;

consequently, lal(r

a2(~)l ~

cllal(~)lla2(~)l

a.e. in co.

Sect. 10.6]

Ezistence of solutions to the minimization problem

533

This inequality shows that the vectors a 1 ( r and a2(~])) are likewise "uniformly" linearly independent a.e. in w, since cl < 1. Hence there exists c3 > 0 such that

c31a1(r A a2(r

>~ l a l ( r 1 6 2

lallla2[ a.e. in w,

and thus there exists a constant C1 such that the two announced inequalities hold. The vector

a3(1]~) -- a 3 ( r

-- lal(~))A a2(r

is thus well defined a.e. in w. Consequently, ba[3(~b) - Oa[3~b"

a3(r

C L2(W),

since la3(r : 1 a.e. in w. The vectors a a ( r are likewise well defined and "uniformly" linearly independent a.e. in w. (iii) Let r e H2(w) be such that aa[3(~b) - aa/3 a.e. in w. Then r C wl'~176 and there exists C2 such that < C2 for all r E I-I2(w).

[0~r

In addition, there exists C3 such that

IIr

0 independent of such fields r such that, for almost all y C w,

IO~r

2

-la~(r

2 = i ~ ( y ) i 2 0; hence, by the generalized Poincard inequality (seer e.g.~ Vol. I~ Thm. 6.1-8), there exists c4 - c4(q, 3'0) such that, for all r E w l ' a ( w ) ,

a

0

Nonlinearly elastic flezural shells

534

[Ch. 10

Let r ~ ,~F (w). Then

A ~ I~1~ ,Zu~2c~A dyandIX ~ c~

0

o

Since the field ~oo 9Vo --->I~3 is continuous on Vo (as the trace on Vo of a function in H2(w); the set ~I'F(w) is not empty by assumption), there exists c5 - c~(c4, C2, ~Oo) such that, for all ~b ~ ~I'F(w),

q(~)

1r + Z IOar

dy < c5.

The Sobolev imbedding w~,q(w) ~ C~ then implies the existence of cs - c6(c5) such that, for all r ~ ~v(w),

and the second assertion is proved. If ~ E ,I,~,(w), the components c9a~r a ~ ( ~ ) of the vector fields c9a/3~ - cDaa~(~) E L~(w) over the vectors a ~ ( ~ ) of the contravariant basis of the tangent plane to the deformed surface ~ ( ~ ) are in L2(w), since a ~ ( ~ ) - c9~ E L~176 by (iii). We next show that these components remain in a bounded subset of the space L2(w) when varies in the set 'I~F(w): (iv) There exists C4 such that

[Oa~" a~(~)10,w _~ C4 for aU ~ E ~F(w). By assumption, 0 E W2'P(w; R 3) with p > 2; as a consequence, Oa~O. 0,,0 E LP(w) C L2(w). Differentiating the relations o~r

o~r = a~(r

- ~

- 0 ~ o . 0~o

in the sense of distributions (which is licit, as is immediately verified) then shows that there exists cz such that, for all ~ C cI'F(w),

1012~" cO2~10,.o_ c7,

Sect. 10.6]

535

Ezistence of solutions to the minimization problem

The relations 011~]J" 0 2 r = (011r

0 2 r + 012r

022r

0 1 r -[- 012r

01~/~ -- (022r

02r

-- 012r

01r

-- 012r

02~]~,

then imply that [011~-~" 02~b[0, w ~ 2C7,

[022r 01r

w ~ 2C7.

Thanks to parts (ii) to (iv), a lower bound for the norms Ib~(r when r C 'I'F(w) can now be established. This lower bound will be essential for proving in part (vii) the coerciveness of the functional IF over the manifold '~F(w). (v)

There exists C5 such that Ib~(r

2O,w >~ 11r 2 W + Cs fo= a11 'r e "I'v(w)

a,/3

Let r e ~F(W). For almost all y e w, the vectors ai(r are linearly independent by (ii), so that the vectors ai(~b)(y) are well defined by the relations ai(r aj(r - ~} for almost all y e w. We can then expand Oa~r as Oa/3~b -- {Oa[3~b. aa(~]J)}a~r(r

+ {Oa/3~b. a3(~.~)}a3(~]J) a.e. in w.

Since bad(C) - 0 a ~ r a3(r la3(r we have, for almost all y E w,

IO~r

2 -I{o~r

a~(r162

1, a n d a 3 ( r

9a a ( ~ b ) -

2 § lb~(r

O,

2

Since the vector fields a ~ ( r lie in a bounded subset of Z~176 when r varies in the set 'I'F(W) (parts (ii) and (iii)) and since the functions Oa~r162 lie in a bounded subset of L 2 (w) when r varies in 'I'v(w) (part (iv)), there exists c8 such that [~0~,

a~(~)}a~(~)[0,~ ~ cs for all ~ E ~I'v(w),

Consequently, there exists c9 such that, for all ~ e 'I'F(w),

a,/3

a,/3

Nonlinearly elastic flezural shells

536

~_ a~0 for all ~p E ~F(w) (see

Since there exists al0 such that llr part (iii)), we finally have w

[Ch. 10

--

,w

w

1,w

c 9 - c20 for all @ E 'I'F(w).

-> ]1r

We now turn our attention to the functional IF. (vi) The functional IF is sequentially weakly lower semi-continuous over the manifold @F(w), i.e.,

r

E ~F(w), l :> 1, and r

___~r E ~F(w) in H2(w)

implies that

Iv(C) _< l i1--+oo minflF(r The weak convergence r

~ r in H2(w) clearly implies that

0af3r '---~ 0af3r in L2(w) and aa(r l) --+ a a ( r

in L2(w),

the last convergences being consequences of the Rellich-Kondra~ov imbedding theorem. We first show that it also implies that a3(r

~ a3(~P) in L2(w).

To this end, we observe that [a3(~bl)] - 1 a.e. in w and that there exists a subsequence ( r m oo of (r I oo such that

since a a ( r

-+ a a ( r

in L2(w). The definition

thus shows that ~(r

A ~2(r

= ~(r

~s m -+ o~

for almost all y E w (by (ii), the vectors aa(r m > 1, and a a ( ~ ) are well defined and "uniformly" linearly independent a.e.

Sect. 10.6]

Ezistence of solutions to the minimizationproblem

537

in w). Therefore, a3(~pm) --4 az(r in L2(w) by Lebesgue's dominated convergence theorem. Since the limit a3(~) is unique, the whole sequence (as(~bt))~l strongly converges in L2(w) to this limit. Using these properties, we next show that

b ~ ( r ~) - ~ r

~3(r

~ a~r

~3(r

- b~(r

in L2(~).

To this end, fix a and ~, let ft E L2(w) denote one component of 0 ~ r t (the same for all l ___ 1), let gt E L~176 denote the same component of a3(~l), and finally, let f E L2(w) and g E L~(w) likewise denote the corresponding components of (gaf~ and a3(~)). In thi~ fashion, the t~o sequ~nce~ ( / ' ) ~ a~d (g~)~=~ ~ti~fy: fl ___xf in L2(w), g! -+ g in L2(w) and Ig'10,oo,~ _< 1 for all l.

It then follows that yg E LZ(w) and

y~9 ~ - / g

i~ LZ(w).

Although these implications are standard, we provide a proof for completeness. For any qo E 79(w), the bilinear form (f, g) E L2(w) • L2(w) -+ f~ .fgqady is strongly continuous; hence f'--~ f in L2(w) and gl _.~ g in L2(w) =~ ~ flgl~ody -4 ~ fg~o dy. Let (/mgm)~= 1 be an arbitrary subsequence of (flgl)~ 1. Since

[fmg~lo,~ < [fm[0,~ and the weakly convergent sequence (.fro)m~176is bounded in L2(w), there is a subsequence (].g.)Oo n--1 of (fmgm)Oo m--1 that weakly converges in Lz(w) to some h E LZ(w). Therefore,

f fngn~d~1-4~hqadY=ffg~ad~tforall~Eg(w), and thus h - fg. Since the limit fg of the subsequence (fngn)n~176 is unique, the whole sequence (y'9~) l~176 = l weakly converges in LZ(w) to this limit. In particular then, we have established that ba#(r t) ~ ba~(~) in L2 (w).

Nonlinearly elastic flezural shells

538

[Ch. 10

We are now in a position to establish the sequential weak lower semi-continuity of IF over '~F(W). Let L2(w) denote the space of all fields of symmetric matrices of order two with components in L2(w). The symmetric bilinear form B" L2(w) x L2(w) --+ R defined by

for all (S, T) - ((Sa~), (ta~)) e L2(w) x L2(w) is strongly continuous and positive definite since there exist constants Cll and cl2 such that 0 < cll and a '~;3'~r(Y)t~rta~ >_ cll

~ Iraqi2 a,~

for all y e ~ and all symmetric matrices (ta~) (Thm. 3.3-2) and -1 0 < cl2 < 1 and 0 < cl2 < %/a(y) < cl2

for all y 6 ~. Being strongly continuous and (strictly) convex, the mapping S 6 L2(w) ~ B(S, S) is thus weakly lower semi-continuous. Let s ta~ "- ba~ (r

_ ba~ and Sa~ "- ba~ ( r

- ba~ .

Then since ba~(r l) ~

ba~(~b)in L~(w), and

thus

B ( S , S) < liminfB(S l, Sl). l--+oo

This shows that the functional IF, which is defined by g3

IF(r

=

%-

for all r C ~F(W) is sequentially weakly lower semi-continuous on 'I'F(w) (recall that L is by assumption a continuous linear form on H2(w)). (vii) There ezist constants C6 and C~ such that 6'6 > 0 and IF(C) > C6[[r

+ C7 for all r c ~ v ( w ) .

Consequently, the functional I v is coercive on the manifold ~V(W).

Ezercises

539

By definition of the functional IF, we have (the constants Cll and c12 appeared in the proof of part (vi))

~3 - c1311r a,/3

where

C13

denotes the norm of the continuous linear form L. Since 1

2

and since, by (v),

ib (r

,~ >__l]r

-4-C5 for a11 r e ~F(w),

the assertion follows, and the existence of a minimizer of the functional IF over the manifold '~F(w) is thus established. II Remarks. (1) The manifold ~F(w) is not convex (save if it contains only one element); cf. Ex. 10.8. (2) A property analogous to that proved in (iii) also holds for isometric three-dimensional manifolds in ]~3; for a precise statement of this property, which is due to Luc Tartar, see, e.g., Vol. I, Ex. 1.16. II

An interesting question consists in identifying the Lagrange multiplier associated with the "constraints" a a ~ ( r aal3 = 0 in w. In this direction, see the formal approach of Fox, Raoult & Simo [1993, Sect. 5.4] in the planar case. EXERCISES

10.1. Let if - (fa) e C3([0, 1]; 1~2) be an injective mapping such that f ' ( t ) ~ 0 for all t e [0, 1] and 3r 1]) is not a segment. Let S - 0(~), where w =]0, 1[• 1[ and O(t, z) = fa(t)e a A- z e 3 for (t, z) E ~. The surface S is thus a portion of a cylinder orthogonal to, and passing through, the planar curve f([0, 1]); cf. Fig. 10.2-1. (1) Assume that 7 0 C { ( 0 , z) C R 2 ; 0 < z < l } U { ( 1 ,

z) E i ~ 2 ; 0 < z < l } .

Nonlinearly elastic flezural shells

540

[Ch. 10

Show that the manifold ~F(W)

= { n = (~i) E W 2 ' 4 ( W ) ; n = O~'n -- 0 on ")'o;

aa/3(r/) -- aao = 0 in w} contains nonzero functions r/. (2) Show that, at each ~ E ,A,tF(w), the tangent space T r to Ji,'tF(w) contains nonzero functions (such a tangent space is defined, e.g., in Sect. 10.2). 10.2. Let :f - (fa) E e3([0, 1];R 2) be an injective mapping such

that f'(~) ~ o fo~ ~II ~ e [0, I]. Let S - 8(~), where w -]0, 1[• 1[ for some 0 < so < 1 and 8(t, s) = s f a ( t ) e a + (1 - s)e 3 for (t, s) C ~. The surface S is thus a portion of a cone with vertex e 3 and passing through the planar curve :f([0, 1]); cf. Fig. 10.2-2. (1) Assume that 7 o - - {(0, s) E R2;so ~_ s 0, coincide with the functions (ba~(y)-ba/3) when r/ corresponds to an inextensional displacement yia i of the middle surface, i.e., when aat3(rl) - aa/3 - 0 in w (Thm. 10.3-1). It is interesting to note that the same functions R~/3(rl) as above have also been proposed by W.T. Koiter (cf. Koiter [1966, eq. (4.11)]), most likely out of different considerations!

Sect. 11.2]

11.2.

Other nonlinear shell theories

OTHER NONLINEAR

549

SHELL T H E O R I E S

Nonlinear "shallow" shell theories are treated separately (see Sect. 11.3.

Naghdi~s nonlinear shell t h e o r y w i t h directors and ext e n s i o n s . While Koiter's theory relies in particular on the KirchhoffLove assumption, Naghdi [1963] has proposed another nonlinear shell theory, in which the a priori assumption on the stresses is the same as in Koiter's, but the a priori assumption of a geometrical nature affords more freedom on the displacements inside the shell; more specifically, the points situated on a line normal to the undeformed middle surface again stay on a line after the deformation has taken place and the distances are unmodified along this line, but this line need no longer remain normal to the deformed middle surface. Unlike Koiter's, Naghdi's theory may thus accommodate shear inside the shell. In this approach, the displacement of any point 0 ( y ) + x~a3(y) inside the undeformed shell is of the form ~e(y) + x~de(y), where ~e (y) _ ~ ( y ) a i ( y ) is the unknown displacement vector of the point O(y) of the middle surface S - 0(~) and de(y) is another unknown vector, called the director at 0(y), that measures the "rotation" of the normal vector after the deformation has taken place. In this fashion, the shell is modeled as a one-director Cosserat surface, whose deformed configuration is specified not only by the displacement field ~ a i 9~ -+ IR3 of the points of the middle surface, but also by a director field d ~ : ~ --+ R 3. This notion is due to Cosserat & Cosserat [1909].

Remark. An example of a one-director Cosserat surface is provided by Naghdi's linear shell theory, with d e - r ae a a as the director field; cf. Sect. 7.4. A planar example is provided by the ReissnerMindlin theory for linearly elastic plates (Vol. II, Sect. 1.9). m After its foundations were properly laid (see notably Naghdi [1963, 1972, 1982], Green, Naghdi & Wainwright [1965], Green & Naghdi [1974], and Reissner [1974]), Naghdi's theory has undergone significant developments, often under the appellations of multi-director shell theories or geometrically ezact shell theories.

550

Koiter's equations and other nonlinear shell theories

[Ch. 11

In these directions, see in particular the illuminating introduction to such theories given in Antman [1995, Chap. 14]. See also Basar [1987], Basar & Kr/itzig [1988], Antman [1989], Simo & Fox [1989], Simo, Fox & Rifai [1989, 1990a, 19905], Fox & Simo [1992], Antman [1997], Valid [1995]; Ge, Kruse & Marsden [1996], Kirchg/issner & Djurdjevic [1997], Djurdjevic [1999] for time-dependent nonlinearly elastic shells; and Basar, Ding & Schultz [1993], Kriitzig [1993], Sasar gr Ding [1995] for the modeling of multi-layered, or laminated, nonlinearly elastic shells by multi-director theories. " F i r s t - o r d e r " a n d " h i g h e r - o r d e r " shell theories. Shell theories, linear and nonlinear, have often been elaborated by assuming that the ratio of 6 to the smallest absolute value of the radii of curvature of the middle surface is also a "small" parameter (for instance the linear Novozhilov and nonlinear Donnell-Mushtari-Vlasov models for shallow shells can be derived in this manner; cf. Sects. 7.6 and 11.3). A shell theory obtained in this fashion is deemed "of the first order" if all terms of order _ 2 with respect to ?7 are neglected in the various formal asymptotic expansions considered and "of a higher order" otherwise. This approach, which leads to theories that are often scarcely distinguishable from the one-director or multi-director theories mentioned supra, is frequently used for modeling multi-layered, or laminated, shells, whose constituting elastic material is thus anisotropic. See notably Librescu [1975], Kriitzig [1974, 1976], Basar & Kriitzig [1985], Ambartsumian [1991], Simmonds [1992], Pomp [1996]. N o n l i n e a r shell t h e o r i e s b a s e d on t h e m e t h o d of internal c o n s t r a i n t s . Another approach advocated by P.M. Naghdi (see notably Green, Laws & Naghdi [1968] and Green & Naghdi [1970]) for generating nonlinear shell theories consists in directly incorporating ad hoc internal constraints in the three-dimensional equations. For instance, the KirchhoJf-Love assumption can play the r61e of such an internal constraint, imposed a priori on the admissible displacements (in its linearized version, this is the approach of Podio-Guidugli [1990]; cf. Sect. 7.5). Special care must be exercised, however, as serious inconsistencies arise if the Lagrange multipliers associated with such internal constraints (in the sense of optimization theory) are not properly

Sect. 11.2]

Other nonlinear shell theories

551

interpreted. Such inconsistencies have been neatly clarified by Antman & Marlow [1991], who showed that the Lagrange multipliers are "reactive" stresses that maintain the constraints, while ad hoc "active" stresses must be added to them so as to make up the total stresses (which are no longer given by constitutive equations); see also Antman [1995, Chap. 14].

Time-dependent nonlinear shell theories can likewise be developed by the method of internal constraints; see Antman [1995, Chap. 14] and Lembo [1996].

A nonlinear Budiansky-Sanders t h e o r y . Destuynder [1982, 1983] has proposed a nonlinear Budiansky-Sanders theory, where the B S (Y) of the "modified linearized change of covariant components Pa~ curvature tensor" are the same as in the linear Budiansky-Sanders theory (Sect. 7.5) and the covariant components

1 a a~ (17) - -~( aa~ ( ~ ) -- aaf3 ) 1 (aZr - 'Ta,o ('r/) + ~ r/o.lla'r/.,-II~ § 'r/311ar/311~) of the change of metric tensor (see, e.g., Thm. 9.1-1) are replaced by the shorter functions

Nonlinear terms thus only appear in the "membrane" part of the strain energy. P. Destuynder then establishes an existence theorem for the associated minimization problem, provided the Christoffel symbols of the middle surface are small enough or an ad hoc geometric assumption is satisfied. His proof makes an essential use of the inequality of Korn's type on a general surface (Thm. 2.6-4). " I n t r i n s i c " n o n l i n e a r shell t h e o r y . The intrinsic approach of Delfour & Zol~sio [1995], which is based on a "tangential differential calculus" and on the "oriented distance function" (Sect. 7.4), has been recently extended to the modeling of nonlinearly elastic shells by Delfour & Zhao [1999].

552 11.3.

Koiter's equations and other nonlinear shell theories NONLINEAR

SHALLOW

[Ch. 11

SHELL THEORIES

Nonlinear shallow shell theories in Cartesian coordinates are already treated in Vol. II, Sects. 4.14 and 5.12. Accordingly, the additional commentary and bibliographical notes found in this section concern mostly nonlinear shallow shell theories expressed in curvilinear coordinates. We recall that, according to the definition proposed and justified by a formal asymptotic method by Ciarlet & Paumier [1986], an elastic shell is deemed "shallow" if, in its reference configuration, the deviation of its middle surface from a plane is of the order of the thickness. More specifically, there exists a smooth enough function 0 :-~ --~ I~ independent of ~ such that

S ~ = 0e(~), where

0e(Yl, Y2) = (Yl, Y2, sO(y1, Y2)) for all (Yl, Y2) C ~.

A w o r d of c a u t i o n . As in the linear case, this specification of how the middle surface should "vary with e" thus also constitutes an assumption on the data, specific to shallow shell theory. II The two-dimensional equations of nonlinearly elastic shallow shells in curvilinear coordinates have been justified by Busse [1995, 1997, 1999] and Andreoiu-Banica [1998, 1999], Andreoiu [1999b] by means of the method of formal asymptotic expansions. S. Busse has considered the case of a clamped shallow shell, while G. Andreoiu has identified Marguerre-von Kdrmdn equations in curvilinear coordinates for a specific class of boundary conditions (introduced by Ciarlet [1980] in the plane case). Since the asymptotic justification and the existence theory for such equations essentially resemble those for the equations of nonlinearly shallow shells in Cartesian coordinates (Vol. II, Sects. 4.14 and 5.12), they are not incorporated into this volume. To give a flavor of these theories, we simply record the twodimensional equations of a nonlinearly elastic clamped shallow shell in curvilinear coordinates, expressed here as a minimization problem:

Sect. 11.3]

553

Nonlinear shallow shell theories

Let

bal3~r, e :__

4Ae#~

Ae + 2# e

F

+

fi, e dx~ + h~ e + h i'e_

p$~ e ~ ._

q~,~ := f~ Sh' ~

+

x~3]o,,~dxe3 + e(h~ 'e

_

1

1

and let a z, ~ designate the vectors of the contravariant bases along the middle surface S e. Then the unknown ~ - (i~), where the functions ~ 9~ -~ I~ are the covariant components of the displacement field ~ a z'e of the middle surface S e, minimizes the energy j sh, e defined by o

{ eba/3~r, eEsh, ~,

, ,~sh, e

} dy

+_~e3ba~crr, e 0err ~]30a~ T~3

over the space (the same space as for Koiter's linear equations; cf. Sect. 7.1)VK(W) := { ~ 7 - (Yi) e H l ( w ) •

Y i - 0~?~3 --0 on 70}-

An inspection of this minimization problem immediately reveals a strong resemblance with the minimization problem found for the "same" nonlinearly elastic shallow shell, but where the unknowns are the Cartesian components of the unknown displacement field (Vol. II, Sect. 4.14). As in the linear case (Sect. 7.6), the resulting theory is more reminiscent of a plate theory than of a shell theory! Using a different definition of "shallowness", requiring in particular that the absolute value of the radii of curvature be everywhere on the middle surface "sufficiently large", Koiter [1966, eqs. (11.43) to (11.50)] also obtains a nonlinear shallow shell theory in curvilinear coordinates, which takes the following form when it is expressed as a

554

Koiter's equations and other nonlinear shell theories

[Ch. 11

minimization problem: The unknown ~e = (~), where the functions ~ : ~ -+ R are the covariant components of the displacement field of e the middle surface, should minimize the energy J.sh, g defined by

g fwaa~ar'e

sh

sh

~3 ~ a a/3~r' +--6en31~rrl3ta~3 V~ dY

- ~pi,"rli~dy , where

sh

9-

+

1 0a~730~73 and

9-

0

,73

-

over the space (again the same as for Koiter's linear equations): VK(W) "= {y = (r/i) e Ht(w)•215

r l i - 0vrl3 = 0 on 70)-

Using the theory of pseudo-monotone operators developed by Lions [1969], Bernadou & Oden [1981] have established the existence of a solution to the associated variational problem if the tangential components of the applied forces and the curvature of the middle surface are "sufficiently small". Their approach makes an essential use of the inequality of Korn's type on a general surface (Thm. 2.6-4). Introducing an Airy stress function in curvilinear coordinates and using the same method as in Ciarlet & Rabier [1980] for establishing the existence of a solution to the yon K~rms equations (see also Vol. II, Sect. 5.8; this method is itself an elaboration over Berger [1967, 1977]), Alexandrescu-Iosifescu [1995a] has also shown that the same nonlinear shallow shell model of W.T. Koiter has at least one solution when the applied tangential components of the applied forces vanish. In addition, Alexandrescu-Iosifescu [1995b] has studied the behavior of the solutions to this model when the shell "becomes a plate". The analysis of the eversion problem for shallow shells modeled by the above Koiter equations has been carried out by Geymonat, Rosati & Valente [1989], Podio-Guidugli, Rosati, Schiaffino & Valente [1989], Geymonat & L~ger [1994]. In this direction, see also Paumier [1978a, 1978b], Paumier & Rao [1989].

Sect. 11.3]

Nonlinear shallow shell theories

555

The same nonlinear shallow shell model is also called the DonneUMushtari-Vlasov model, so named by Sanders [1963] after Donnell [1933], Vlasov [1944], and Mushtari-Galimov [1961]. Under this name, it has been justified by Figueiredo [1990a] by means of a formal asymptotic method with two "small" parameters, the thickness 2e and the ratio of e to the smallest absolute value of the radii of curvature of the middle surface. Figueiredo [1990b] has also established the existence of a solution, by means of the implicit function theorem. Other "classical" equations have been likewise deemed appropriate for modeling nonlinearly elastic shallow shells. A thorough treatment of their mathematical properties, together with a detailed discussion of the various a priori assumptions they are based upon, is found in the recent book by Vorovich [1999], which contains in addition an extensive list of references from the Russian literature on shell theory. The modeling of nonlinearly elastic shallow shells lying on an obstacle leads to interesting "unilateral eigenvalue problems", which can be solved by means of pseudo-monotone operator theory as shown by Gratie [1998, 1999a, 1999b]. In this direction, see also Goeleven, Nguyen & Th~ra [1993a, 1993b], Goeleven [1996], Gratie & Pascali [1997, 1999], Pauchard, Pomeau & Rica [1997], Le & Schmitt [1997], Goeleven & Motreanu [1998].

This Page Intentionally Left Blank

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SOKOLOWSKI, J.; ZOL]~SIO, J.P. [1992]: Introduction to Shape Optimization: Shape Sensitivity Analysis, Springer-Verlag, Heidelberg. SPIVAK, M. [1975]: A Comprehensive Introduction to Differential Geometry, Volumes I to V, Publish or Perish, Boston. SrtUBSHCHIK, L.S. [1968]: Nonstit~ess of a nonshallow spherical dome, J. Appl. Math. Mech. 32, 435-445. SB.UBSHCHIK,L.S. [1972]: On the problem of non-stit~ess in the nonlinear theory of shallow shells, Izv. Akad. Nauk SSSR, .qer. Math., 86, 890-909 (in Russian). SRUBSHCHIK, L.S. [1980]: Precritical equilibrium of a thin shallow shell of revolution and its stability, J. Appl. Math. Mech. 44, 229-235. STEIN, E. [1970]: Singular Integrals and Differentiability Properties of Functions, Princeton University Press. STOKe.R, J.J. [1968]: Nonlinear Elasticity, Gordon and Breach, New York. STOKe.R, J.J. [1969]: Differential Geometry, John Wiley, New York. STOLARSKI, H.; BSr.YrSCHKO, T. [1982]: Membrane locking and reduced integration for curved elements, J. Appl. Mech. 49, 172-176. STOLARSKI, H.; BELYTSCHKO,T.; L~.~., S.H. [1995]: A Review of Shell Finite Elements and Gorotational Theories, in Computational Mechanics Advances, Vol. 2, 125-212. STRUIK, D.J. [1961]: Lectures on Classical Differential Geometry, Second Edition, Addison-Wesley, Reading. STRUW~., M. [1990]: Variational Methods, Springer-Verlag, Berlin. SuRI, M. [1997]: A reduced constraint hp finite element method for shell problems, Math. Gomp. 6 6, 15-29. SuP.x, M.; BABUgKA, I.; SCHWAB, C. [1995]: Locking effects in the finite element approximation of plate models, Math. Gomp. 64, 461-482. SZABO, B.A.; SAHRMANN, G.J. [1988]: Hierarchic plate and shell models based on p-extension, Internat. Y. Numer. Methods Bngrg. 2tl, 1855-1881. SzP.RI, A.J. [1990]: On the everted states of spherical and cylindxical shells, Quart. Appl. Math. 47, 49-58. TARTAR, L. [1978]: Topics in Nonlinear Analysis, Publications Math6matiques d'Orsay No. 78.13, Universit6 de Paris-Sud, Orsay. TP.r.EGA, J.J.; LBWIgrSKI, T. [1998a]: Homogenization of linear elastic shells: Pconvergence and duality. Part I. Formulation of the problem and the effective model, Bull. Polish Acad. Sci., Technical Sci., 46, 1-9. T~.LSGA, J.J.; L~.WIr~SKI, T. [1998b]: Homogenization of linear elastic shells: F-convergence and duality. Part II. Dual homogenization, Bull. Polish Acad. Sci., Technical Sci., 46, 11-21. THOMAS, T.Y. [1934]: Systems of total differential equations defined over simply connected domains, Annals Math. $5, 730-734. TIMOSHENKO, S.P. [1951]: Theory of Elasticity, McGraw-Hill, New York. TIMOSH~.NKO, S.P.; WOINOWSKY-KRI~.G~.R, S. [1970]: Theory of Plates and Shells, McGraw-Hill, New York. TRABUCHO, L.; VxAgro, J.M. [1987]: Derivation of generalized models for linear elastic beams by asymptotic expansion methods, in Applications of Multiple Scalings in Mechanics (P.G. CIARI,ST & E. SANCH~,Z-PAr.~.NCIA,Editors), pp. 302-315, Masson, Paris. TRABUCHO, L.; VIA~O, J.M. [1996]: Mathematical modelling of rods, in Handbook of Numerical Analysis, Vol. I V (P.G. CIARI,ST & J.L. LIONS, Editors), pp. 487-974, North Holland, Amsterdam.

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INDEX

a p r i o r i assumption of" a geometrical or mechanical nature : 336, 363, 546 admissible: applied force : 265, 292, 293, 298, 351 m displacement : 303 inextensional deformation : 530 inextensional displacement: 439, 503 linearized inextensional displacement : 303 analytic functions: 121, 125 anisotropic elastic material : 162, 178, 234, 326, 360, 366, 550 Ansatz of the m e t h o d of formal asymptotic expansions : 164, 413 applied b o d y force : 7, 25, 386 assumptions o n - s : 152, 162,164, 179, 180, 199, 229, 232, 233, 247, 265, 305, 322, 326, 414, 442,443, 458, 507 applied force ( a d m i s s i b l e - - ) : 265, 292, 293, 298, 351 applied surface force : 7, 26, 386 assumptions on m s : 152, 162, 164, 179, 180, 199, 229, 247, 265, 305, 322, 414, 442, 443, 507 area element : 19 area element on a surface : 70 assumptions on the data : See "applied body force", "applied surface force", "Lam~ constants", "shallow shell" justification of m : 162, 425, 443, 476, 507 asymptotic expansions (method of f o r m a l - - ) : 164, 413 asymptotic line : 83, 295 b e n c h m a r k problem : 361 bending: badly-inhibited ~ : 292 not i n h i b i t e d - : 325 w e l l - i n h i b i t e d - : 232 bending in shells : See "flexuxal-dominated behavior", "flexuxal theory", "linearly elastic flexuxal shell", "nonlineafly elastic flexuxal shell" bending m o m e n t : 344 b o d y force : See "applied b o d y force" boundary condition: of place : 8, 32, 387 of pressure : 455 of traction : 388 c o m p l e m e n t i n g - : 123, 236, 237, 373 t w o - d i m e n s i o n a l - s of clamping : 101, 116, 304, 305, 306, 322, 344 two-dimensional m s of simple support : 115, 134, 339, 439, 451, 530 two-dimensional ~ s of strong clamping : 503, 504, 524, 525, 530, 548 t w o - d i m e n s i o n a l - s of weak simple support : 234

Indez

584

b o u n d a r y layer : 351, 362,368, 371, 374

BUDIANSKY-SANDERS linearized change of c u r v a t u r e tensor : 367 BUDIANSKY-SANDERS shell t h e o r y : l i n e a r - - - : 367 nonlinear m : 551 canonical e x t e n s i o n : 144

CARTESIAN c o m p o n e n t s : 6 of the displacement field : 7, 387, 459, 463

CARTESIAN coordinates : 6, 67 GREEN-ST VENANT strain tensor i n : 388 KORN'S inequality i n : See " K o r n ' s inequality" linearized change of metric tensor in m : 9 linearized elasticity i n : 10 linearized strain tensor i n : 9 linearized strains i n : 9, 36 nonlinear elasticity in ~ : 391 thxee-dimensional elasticity tensor in ~ : 11 CARTESIAN frame: 6 CAUCHY-GREEN strain tensor (right m ) : 9 change of c u r v a t u r e tensor on a surface : 508, 519, 524, 548 change of c u r v a t u r e tensor on a surface (linearized ~ ) 308, 322, 338, 344 BUDIANSKY-SANDERS ~ : 367 NAGHDI'S ~ : 366

: 93, 174, 181,

change of m e t r i c tensor in a t h r e e - d i m e n s i o n a l d o m a i n : in CARTESIAN coordinates : 388 in curvilinear coordinates : 398 change of m e t r i c tensor in a three-dimensional d o m a i n (linearized m ) : ill CARTESIAN coordinates : 9 in curvilinear coordinates : 36 change of m e t r i c tensor on a surface : 437, 450, 524, 548 change of m e t r i c tensor on a surface ( l i n e a r i z e d - - ) : 91, 170, 181,210, 228, 308, 321,338, 344, 366

CHRISTOFFEL symbols : 29, 33 of the first kind : 55, 60 of t h e second kind : 55, 60

CHRISTOFFEL symbols on a surface : 88, 136 of the first kind : 130 of the second kind : 130 clamping : two-dimensional b o u n d a r y conditions o f - - : 101,116, 304, 305, 306, 322, 344 two-dimensional b o u n d a r y conditions of strong ~ : 503, 504, 524, 525, 530, 548 CODAZZI-MAINARDI i d e n t i t i e s : 131, 133 coerciveness

of

a

f u n c t i o n a l : 431, 452, 466, 538

c o m p l e m e n t i n g b o u n d a r y condition : 123, 236, 237, 373 c o m p o s i t e m a t e r i a l (shell m a d e with a ~ ) cone : 296, 305, 329, 505, 540

: 368, 371

Indez

585

constitutive equation : three-dimensional: 389 two-dimensional: 229, 451 c o n t i n u a t i o n t h e o r e m ( u n i q u e m ) : 125, 126, 294 c o n t r a v a r i a n t basis : 21 c o n t r a v a r i a n t basis on a surface : 86 of t h e t a n g e n t p l a n e : 72 contravariant - - of of of of of of of w of of of of - -

- -

- -

components 9 a v e c t o r : 56 t h e a p p l i e d b o d y force d e n s i t y : 25 t h e a p p l i e d surface force d e n s i t y : 26 t h e first PIOLA-KIRCHHOFF stress t e n s o r : 403 t h e l i n e a r i z e d stress t e n s o r : 38 t h e m e t r i c t e n s o r : 20, 57 t h e m e t r i c t e n s o r of a surface : 72 t h e r e s u l t a n t stress t e n s o r : 224 t h e s e c o n d PIOLA-KIRCHHOFF stress t e n s o r : 402 t h e t h r e e - d i m e n s i o n a l e l a s t i c i t y t e n s o r : 32 t h e t w o - d i m e n s i o n a l e l a s t i c i t y t e n s o r of a shell : 101

c o n t r o l l a b i l i t y of shells : 234, 3 6 1 , 3 7 1 convergence : of d i s p l a c e m e n t s : 183, 209, 231, 233, 268, 291, 308, 324, 370, 461 of stresses : 234, 237, 326, 331 F-: 233, 326, 459 c o o r d i n a t e line : 17 on a surface : 68 c o o r d i n a t e s (see also "CArtTSSXAN c o o r d i n a t e s " a n d " c u r v i l i n e a r c o o r d i n a t e s " ) : cylindrical--: 15 s p h e r i c a l u : 15, 67 s t e r e o g r a p h i c ~ : 67 COSSErtAT surface (one d i r e c t o r - - )

: 363, 549

c o v a r i a n t b a s i s : 17 of t h e t a n g e n t p l a n e : 69 on a surface : 86 - -

covariant components : of a v e c t o r : 25, 56 of t h e c h a n g e of m e t r i c t e n s o r : 398 - - of t h e c u r v a t u r e t e n s o r : 81 - - o f t h e d i s p l a c e m e n t f i e l d : 25 of t h e d i s p l a c e m e n t field of a surface : 86 - - of t h e GRSEN-ST VBNANT s t r a i n t e n s o r : 397 of t h e l i n e a r i z e d c h a n g e of c u r v a t u r e t e n s o r : 93 of t h e l i n e a r i z e d c h a n g e of m e t r i c t e n s o r : 36 of t h e l i n e a r i z e d c h a n g e of m e t r i c t e n s o r on a surface : 91 of t h e l i n e a r i z e d s t r a i n t e n s o r : 36 of t h e m e t r i c t e n s o r : 18, 57 of t h e m e t r i c t e n s o r of a surface : 69 - -

covariant derivative: a t e n s o r field : 38, 94, 133, 224, 402 - - of a v e c t o r field : 30, 33, 451 - - of a v e c t o r field on a surface : 88 s e c o n d order ~ : 94, 345 -

-

o

f

Indez

586

c u r v a t u r e (see also " c u r v a t u r e t e n s o r on a surface") : center o f - - : 7'4, ?7 - - o f a p l a n a r curve : ?5, 76 G A U S S I A N - : 82, 83, 84, 121, 133 line o f : 82 mean: 82 p r i n c i p a l u : 82 principal radius of: 82 r a d i u s o f - - : 74 total: 82 cuxvatuxe t e n s o r on a surface : c o v a r i a n t c o m p o n e n t s of t h e : 81 m i x e d c o m p o n e n t s of t h e : 81 RIEMANN u : 136 cuxvilinear c o o r d i n a t e s : 15 GREEN-ST VENANT s t r a i n t e n s o r i n : 397 KORN's i n e q u a l i t y i n : 44, 48, 53, 59 l i n e a r i z e d change of m e t r i c t e n s o r i n : 36 l i n e a r i z e d elasticity i n : 3? l i n e a r i z e d s t r a i n t e n s o r i n - - : 36 l i n e a r i z e d strains i n : 36 n a t u r a l - - for a shell : 14, 145 n o n l i n e a r elasticity i n : 392 t h r e e - d i m e n s i o n a l e l a s t i c i t y t e n s o r in - - : 32 cuxvilinear c o o r d i n a t e s on a surface : 65 c y l i n d e r : 296, 328, 440, 465, 504, 539 circular ~ : 66, 191 c y l i n d r i c a l c o o r d i n a t e s : 15 d e f o r m a t i o n : 9 , 3 8 ? , 456 a d m i s s i b l e i n e x t e n s i o n a l - : 530 large - - n o n l i n e a r flexuxal shell t h e o r y : 525 large - - n o n l i n e a r m e m b r a n e shell t h e o r y : 452, 463 s c a l e d - - : 458 d e f o r m a t i o n g r a d i e n t : 10 d e f o r m e d c o n f i g u r a t i o n : 9, 287 d i r e c t o r field on a surface : 363 d e v e l o p a b l e surface : 83 d~velopp~e : 75 d i r e c t o r shell t h e o r y : m u l t i - - - : 549 o n e - - - : 363, 549 displacement : admissible-

: 303, 439, 503

CARTESIAN c o m p o n e n t s of t h e -

: ?, 387, 459 convergence of t h e s : 183, 209, 231, 233, 268, 291, 308, 324, 370, 461 c o v a r i a n t c o m p o n e n t s of t h e : 25 c o v a r i a n t c o m p o n e n t s of t h e - - of a surface : 86 field in t h r e e - d i m e n s i o n a l e l a s t i c i t y : ? m field of a surface : 86 error e s t i m a t e s f o r - s : 233, 350, 351, 358, 360 i n e x t e n s i o n a l - - : 439, 503

Indez

587

limit ~ s : 226, 232, 289, 319, 447, 462, 522 linearized inextensional ~ : 162 n o r m a l u of the middle surface : 232, 325 scaled m s : 152, 199, 246, 303, 408, 458 t a n g e n t i a l m of the middle surface : 232, 325 d i s p l a c e m e n t gradient : 10, 389 d i s p l a c e m e n t - t r a c t i o n p r o b l e m : 390 l i n e a r i z e d - - : 10 d o m a i n in R n : 6, 40 DONNELL-MUSHTARI-VLASOV nonlinear shallow shell t h e o r y : 555 e d g e : See "fold" eigenvalue p r o b l e m s for shells : 234, 326, 358, 371 u n i l a t e r a l m : 555 elastic m a t e r i a l : anisotropic m : 162, 178, 234, 326, 360, 366 homogeneous: 6, 388 isotropic u : 6, 388 linearly m : See "linearized elasticity" nonhomogeneous: 162, 178, 234, 326, 360, 366 n o n l i n e a r l y - : 389, 392, 454 soft ~ : 464 ST VENANT-KIRCHHOFF ~ : 389, 392, 430, 455 elasticity tensor : t h r e e - d i m e n s i o n a l - in CARTESIAN coordinates : 11, 392 t h r e e - d i m e n s i o n a l ~ in curvilinear coordinates : 32, 57 t w o - d i m e n s i o n a l R of a s h e l l : 101, 117, 228, 291,322, 338, 344, 365, 450, 527 e l a s t o d y n a m i c s for a shell : See " t i m e - d e p e n d e n t equations" e l l i p s o i d : 121, 197, 297 elliptic m e m b r a n e shell (linearly elastic R ) : See "linearly elastic elliptic m e m b r a n e shell" elliptic m i d d l e surface (shells with ~ )

: 120, 196, 293

elliptic p o i n t : 83 elliptic s u r f a c e : 120, 122, 126, 130, 196 elliptic s y s t e m : s t r o n g l y ~ : 236, 373 u n i f o r m l y ~ : 123, 236, 237, 373 energy : See also " t h r e e - d i m e n s i o n a l energy", "two-dimensional energy", " t w o - d i m e n s i o n a l strain energy '~ existence of a m i n i m u m : 224, 228, 290, 321, 339, 340, 3 9 1 , 4 6 2 , 530, 551 m i n i m i z e r of an ~ : See " m i n i m i z a t i o n of a functional" stored ~ f u n c t i o n : 391, 392 strain ~ : See "two-dimensional strain energy" e q u a t i o n s of e q u i l i b r i u m : in CARTESIAN coordinates : 387 in curvilinear coordinates : 403 linearized m in CARTESIAN coordinates : 12 linearized ~ in curvilinear coordinates : 40 t w o - d i m e n s i o n a l - - : 229, 451 error e s t i m a t e s for displacements : 233, 350, 351, 358, 360

Indez

588 EUCLIDEAN space : three-dimensional ~ e three-dimensional- : 5

: 5

EUL~.R characteristic of a surface : 83 eversion of shells : 442, 542, 554 existence of solutions : 52, 101, 111, 115, 126, 223, 317, 338, 340, 366, 367, 376, 392, 452, 453, 529, 551, 554 face of a shell : lateral - - : 146 lower - - : 148 u p p e r m : 148 f l e x u r a l - d o m i n a t e d behavior : 361 flexural shell (linearly elastic ~ )

: See "linearly elastic flexural shell"

flexural shell (nonlinearly elastic - - ) : See "nonlinearly elastic flexural shell" flexural t h e o r y : See "shell t h e o r y " f o l d : 76, 295, 296, 297 force : See "applied b o d y force", "applied force", "applied surface force" formal a s y m p t o t i c e x p a n s i o n : 164, 414 leading t e r m in a - - : 164, 414 m e t h o d of m s : 164, 413 t e r m of order q in a : 141 frame-indifferent flexural t h e o r y : 525, 541 frame-indifferent m e m b r a n e t h e o r y : 452, 463, 466 functional (see also "energy" a n d " m i n i m i z a t i o n of a functional") : coerciveness of a : 431, 452,466, 538 as a F-limit : 460 s t a t i o n a r y point of a : 399, 445, 448, 520 weak lower semi-continuity of a : 431, 452, 536 f u n d a m e n t a l form of a surface : f i r s t - : 69, 72 s e c o n d - : 81 third: 99 I~-convergence : 233, 326, 459 F - l i m i t : 460

GAuss:

formula o f - : 88 T h e o r e m a egregium o f - - : 131, 136

GAUSS-BONNET t h e o r e m : 83, 133

GAUSSIAN c u r v a t u r e : 82, 83, 84, 121, 133 generalized m e m b r a n e shell (linearly elastic - - ) : See "linearly elastic generalized m e m b r a n e shell" genus of a surface : 83 g e o m e t r i c a l l y exact shell t h e o r y : 549

GREEN-ST VENANT strain tensor : - - i n CARTESIAN coordinates : 388 --- in curvilinear coordinates : 397 hierarchic shell t h e o r y : 368 HILBERT uniqueness m e t h o d (HUM) : 361

589

Indez

HOLMGI%EN'S uniqueness t h e o r e m : 124 h o m o g e n e o u s elastic m a t e r i a l : 6, 3 8 8 h o m o g e n i z a t i o n of shell equations : 234, 360 h y p e r b o l i c middle surface (shells w i t h - - )

: 295, 362

h y p e r b o l i c p a r a b o l o i d : 132 h y p e r b o l i c point : 83 h y p e r b o l o i d of revolution : 294 hyperelastic m a t e r i a l : 391, 392, 454 implicit function t h e o r e m : 144, 392, 453, 555 inextensional d e f o r m a t i o n : 530 inextensional displacement : 439, 503 l i n e a r i z e d - : 162, 303 infinitesimal rigid displacement : 46 on a surface : 109, 115 infinitesimal rigid displacement l e m m a : 49 o n a general surface : 109, 366, 377 on a general surface with little regularity : 114 N on an elliptic surface : 122, 295 infinitesimal rigidity of a surface : 297 infinitesimal r o t a t i o n field : 133 interior layer : 362 internal constraints ( m e t h o d o f - - ) : 368, 550 intrinsic shell t h e o r y : l i n e a r - : 368 n o n l i n e a r - : 551 isometric s u r f a c e s : 85, 439, 441, 531 isotropic elastic m a t e r i a l : 6, 3 8 8 j u n c t i o n s b e t w e e n shells : 360, 454 KII%CHHOFF-LOVE a s s u m p t i o n : 336, 372, 546, 550 l i n e a r i z e d - : 336, 360, 368, 372 KIB.CHHOFF-LOVE plate t h e o r y : 227, 320, 328 KOITER energy : 344, 548 KOITER s t r a i n energy 9 344, 548 KOIT~.I~'s linear shell equations : 100, 111, 115, 337, 339, 341, 344, 360, 373, 375 admissible applied forces for - - : 351 eigenvalue p r o b l e m for - - : 358 for shells whose middle surface has little regularity : 115, 339, 362 t i m e - d e p e n d e n t - : 347, 361 KOITER'S nonlinear shallow shell equations : 553 KOITER'S nonlinear shell equations : 547 KORN's inequality : in CARTESIAN coordinates : 49, 113, 207, 217, 253, 257 in curvilinear coordinates : 44, 48, 53, 59

590

Indez

KORN'S type (inequality o f - - ) : on a general surface : 103, 111, 118, 134, 318, 339, 356, 377, 551, 554 w on a general surface with little regularity : 115, 340 on an elliptic surface : 126, 197, 208, 216, 225, 261, 349 t h r e e - d i m e n s i o n a l - for a family of linearly elastic elliptic membrane shells : 205, 212, 220, 221 three-dimensional m for a family of linearly elastic shells : 259, 269,

271, 310 LAGRANGE multiplier: 319, 539, 550 LAMI~ constants : 7, 389 assumptions on the ~ : 152, 162, 199, 229, 247, 303, 322, 442, 443, 507 laminated shell : 368, 550 large deformation, or large displacement, flexural theory : 525 large deformation, or large displacement, membrane theory : 452, 463 lateral face of a shell : 146

LAX-MILGRAM lemma : 54, I01, I17, 192, 225, 278, 285, 288, 319, 339 layer : b o u n d a r y w : 351, 362, 368, 371, 374 i n t e r i o r - : 362 length element : 20 length element on a surface : 70 limit displacements : 226, 232, 289, 319, 447, 462, 522 limit stresses : 234, 237, 326, 331,452, 546 line of curvature : 82 linear shell theory : See "shell theory" linearization trick : 415 linearized change of curvature tensor : 93, 174, 181, 308, 322, 338, 344, 526 BUDIANSKY-SANDERS - - : 367 NAGHDI'S ~ : 366 linearized change of metric tensor in a three-dimensional domain : in CARTESIAN coordinates : 9, 36 m in curvilinear coordinates : 36 linearized change of metric tensor on a surface : 91, 170, 181, 210, 228, 308, 321, 338, 344, 366, 452, 526 linearized elasticity (three-dimensional--) : in CARTESIAN coordinates: 8, 10, 455 in curvilineax coordinates : 32, 38, 52 linearized inextensional displacement : 162, 303 linearized KIRCHHOFF-LOVE assumption : 336, 360, 368, 372 linearized rotation field : 364, 376 linearized strain (see also "change of metric") 9 in CARTESIAN coordinates : 9 in curvilinear coordinates : 36 M tensor : 9 s c a l e d - - : 153

Indez

591

linearized stress in CARTESIAN c o o r d i n a t e s : 11 in curvilinear coordinates : 38 linearized t r a n s v e r s e shear s t r a i n tensor : 366 linearly elastic elliptic m e m b r a n e shell : definition of a m : 196 e x a m p l e of a - - : 197 KOITBR'S e q u a t i o n s for a : 347 t w o - d i m e n s i o n a l constitutive equations for a : 229 t w o - d i m e n s i o n a l e n e r g y of a : 224, 229 t w o - d i m e n s i o n a l equations of a ~ : 117, 126, 210, 223, 227, 359 t w o - d i m e n s i o n a l equilibrium equations for a : 229 t w o - d i m e n s i o n a l s t r a i n energy of a ~ : 229 linearly elastic flexural shell : 111, 541 definition of a : 199, 302 e x a m p l e of a m : 303, 304, 305, 328, 329, 330 KOITER'S equations for a u : 355 t w o - d i m e n s i o n a l e n e r g y of a : 322 t w o - d i m e n s i o n a l equations of a : 101, 309, 318, 320, 359 t w o - d i m e n s i o n a l s t r a i n energy of a ~ : 322 linearly elastic generalized m e m b r a n e shell : admissible applied forces for a ~ : 265, 292, 293, 298 definition of a ~ : 245 e x a m p l e of a - - : 293, 294, 295, 296, 297 of t h e first k i n d : 262, 268, 293 of t h e second k i n d : 262, 283, 293 KOITER'S e q u a t i o n s for a ~ : 351 t w o - d i m e n s i o n a l energy of a ~ : 290 t w o - d i m e n s i o n a l equations of a : 268, 283, 359 t w o - d i m e n s i o n a l s t r a i n energy of a ~ : 290 linearly elastic m a t e r i a l : See "linearized elasticity" linearly elastic m e m b r a n e shell : 199, 246, 466 linearly elastic shallow shell : definition of a ~ : 369, 371 t w o - d i m e n s i o n a l e n e r g y of a -

: 370

LIONS ( l e m m a of J.L. ~ ) : 42, 105, 119, 218, 256, 279, 376 locking: p h e n o m e n o n : 362, 366 membrane: 362, 366, 368 lower face of a shell : 148 m a n i f o l d : 439, 472, 502, 520, 526, 529, 542, 543 t a n g e n t space to a : 472, 503, 520 MAB.GUERRE-VON K.~RM~N equations in curvilinear coordinates : 552 m e a n c u r v a t u r e : 82 m e m b r a n e - d o m i n a t e d b e h a v i o r : 361 m e m b r a n e locking : 362, 366 m e m b r a n e shell (linearly elastic ~ ) : See "linearly elastic elliptic m e m b r a n e shell", "linearly elastic generalized m e m b r a n e shelr'~ "shell t h e o r y " m e m b r a n e shell (nonlinearly e l a s t i c - - ) : See "nonlinearly elastic m e m b r a n e shell" m e m b r a n e t h e o r y : See " p l a n a r m e m b r a n e t h e o r y " , "shell t h e o r y "

592

Indez

m e t r i c tensor : 55 contravariant c o m p o n e n t s of t h e : 19 covariant c o m p o n e n t s of the ~ : 18 m i x e d c o m p o n e n t s of the ~ : 57 m e t r i c tensor on a surface : contravariant c o m p o n e n t s of the ~ : 72 covariant c o m p o n e n t s of the ~ : 69 m i d d l e surface of a shell : 143 with folds : 76 with little regularity : 76, 114, 115, 339, 362, 366 with no b o u n d a r y : 143, 234, 292, 297 m i n i m i z a t i o n of a functional : 224, 228, 290, 321, 339, 340, 391, 446) 448, 452, 456, 462, 520, 523, 529, 553 mixed component : of the c u r v a t u r e tensor on a surface : 81 of the metric tensor : 57 multi=dixector shell t h e o r y : 549 m u l t i -l a y e re d shell : 368, 371,454, 550 multiplicity of solutions : 530 NAGHDI'S linear shell equations : 365, 376 for shells whose middle surface has little regularity : 366 NAGHDI's linearized change of curvature tensor : 366 NAGHDI'S nonlinear shell t h e o r y : 549 n a t u r a l curvilinear coordinates for a shell : 14, 145 n a t u r a l s t a t e : 6, 388 n o n h o m o g e n e o u s elastic m a t e r i a l (shell m a d e with a - - ) 326, 360, 366

: 162, 178, 234,

nonlinear elasticity ( t l a r e e = d i m e n s i o n a l - - ) : - - i n CARTESIAN c o o r d i n a t e s : 391 in curvilinear coordinates : 392 nonlinear p l a n a r m e m b r a n e t h e o r y : 451,453, 454, 460 non l i n e a r shell t h e o r y : See "shell theory" nonlineaxly elastic flexural shell : definition of a - - : 502 e x a m p l e of a : 504, 505, 506, 539, 540 two-dimensional energy of a - - - : 524 two-dimensional equations of a : 518, 522, 523 two-dimensional strain energy of a : 524 n o n l i n e a r l y elastic m a t e r i a l : 389, 392, 454 n o n l i n e a r l y elastic m e m b r a n e shell (theory derived by formal analysis) : definition of a : 439 e x a m p l e of a m : 440, 4 4 1 , 4 6 5 two-dimensional constitutive equations for a : 451 two-dimensional energy of a : 445, 446, 450 two-dimensional equations of a --- : 444, 448, 450 two-dimensional equilibrium equations for a : 451 two-dimensional strain energy of a : 450

Indez n o n l i n e a r l y elastic m e m b r a n e shell (theory derived by P-convergence) : stored energy function of a : 463 two-dimensional energy of a : 463 n o n l i n e a r l y elastic shallow shell: definition of a : 552, 553, 555 t w o - d i m e n s i o n a l energy of a : 553, 554 n o n u n i q u e n e s s of solutions : 530 NOVOZHILOV'S shell t h e o r y : 371 n u m e r i c a l a p p r o x i m a t i o n of shell problems : 362, 363, 368 obstacle (shell lying on a n - - ) : 555 one-director COSSBRAT surface : 363, 549 one-director shell t h e o r y : 363, 549 parabolic m i d d l e surface (shells w i t h - - ) : 296 parabolic p o i n t : 83 PIOLA-KIRCHHOFF stress tensor ( ~ s t - - ) : 388, 403 PIOLA-KIRCHHOFF stress tensor ( s e c o n d - - ) : 387 p l a n a r m e m b r a n e t h e o r y ( n o n l i n e a r - - ) : 451,453, 454, 460 p l a n a r p o i n t : 82, 132 p l a t e : 306, 329, 4 6 5 , 5 0 6 shell b e c o m i n g a : 192, 234, 326, 358, 375 p l a t e t h e o r y : 152, 326, 358, 370 KII%CHHOFF-LOVE: 227, 320, 328 KEISSNER-MINDLIN- : 363, 549 p o i n t on a surface : e l l i p t i c - : 83 h y p e r b o l i c - : 83 parabolic: 83 planar: 82, 132 u m b i l i c a l - : 82, 133 POISSON ratio : 389 p o l y c o n v e x stored energy function : 392 pressure l o a d : 455 principal c u r v a t u r e : 82 principal d i r e c t i o n : 82 principal radius of c u r v a t u r e : 82 principle of v i r t u a l work : l i n e a r i z e d - in CARTESIAN c o o r d i n a t e s : 11 l i n e a r i z e d - in curvilinear coordinates : 40 in CARTESIAN c o o r d i n a t e s : 388 - - in curvilinear coordinates : 403 quasiconvex : envelope : 459, 462 function : 459 -

-

reference configuration : 6, 386 of a shell : 12, 143 r e g u l a r i t y of solutions : 60, 122, 235, 341, 373 P~EISSNER-MINDLIN p l a t e t h e o r y : 363, 549 RIEMANN c u r v a t u r e tensor on a surface : 136

593

594

Indez

rigid displacement l e n u n a : See "inFinitesimal rigid displacement", "infinitesimal rigid displacement l e m m a " rigidification of a surface : 297 rigidity of a surface : 442 i n f i n i t e s i m a l - : 297 r o t a t i o n field : infinitesimal u : 133 l i n e a r i z e d - - : 364, 376 scaled s t r a i n : See "strain" scaled t l ~ e e - d i m e n s i o n a l elasticity tensor of a shell : 154, 410 scaled t l ~ e e - d i m e n s i o n a l equations : for a linearly elastic shell : 154 - - for a nonlinearly elastic shell : 410 scaled two-dimensional elasticity tensor of a shell : 158, 170, 181, 210, 308, 430 scaled u n k n o w n : See "scalings of displacements" scaled vector field: 152, 408 scalings of deformations : 458 scalings of displacements : 152, 199, 246, 303, 408, 458 justification o f - - : 162, 415 scalings of stresses : 237 sensitive variational p r o b l e m : 293, 295, 296 shallow shell : a s s u m p t i o n on the middle surface of a - - : 369, 371, 552 linearly e l a s t i c - : 369 n o n l i n e a r l y e l a s t i c - : 552 shape o p t i m i z a t i o n for shells : 361 shear : linearized t r a n s v e r s e - - tensor : 366 shell (see also "shallow shell") : 12, 143 b o u n d a r y layer in a : 351, 362 c l a m p e d u : 101, 116, 146, 339 controllability of m s : 234, 361 eigenvalue p r o b l e m for - - s : 234, 326, 358, 3 7 1 , 5 5 5 eversion o f - - s : 442, 542, 554 h o m o g e n i z a t i o n o f - - e q u a t i o n s : 234, 360 j u n c t i o n s b e t w e e n m s : 360, 454 laminated: 368, 550 lateral face of a - - : 146 linearly elastic elliptic m e m b r a n e : See "linearly elastic elliptic m e m b r a n e shell" linearly elastic f l e x u r a l - - - : See "linearly elastic flexural shell" linearly elastic generalized m e m b r a n e - - : See "linearly elastic generalized m e m b r a n e shell" lower face of a : 148 m i d d l e surface of a m : 143 m u l t i - l a y e r e d - - : 368, 371,454, 550 n a t u r a l curvilinear coordinates for a : 14, 145 n o n l i n e a r l y elastic f l e x u r a l - : See "nonlinearly elastic flexural shell" n o n l i n e a r l y elastic m e m b r a n e : See "nonlinearly elastic m e m b r a n e shell"

Indez

595

n u m e r i c a l a p p r o x i m a t i o n of u p r o b l e m s : 362, 363, 368 shape o p t i m i z a t i o n for u s : 361 b e c o m i n g a p l a t e : 192, 234, 326, 358, 375 m a d e w i t h a composite m a t e r i a l : 368, 371 m a d e w i t h a n o n h o m o g e n e o u s m a t e r i a l : 162, 234, 326, 360, 366 m a d e with a soft m a t e r i a l : 464 m a d e w i t h an anisotropic m a t e r i a l : 162, 234, 326, 360, 366, 550 whose m i d d l e surface has little regularity : 76, 114, 115, 339, 362, 366 whose m i d d l e surface has no b o u n d a r y : 143, 234, 292, 297 w i t h folds : 76, 295, 296, 297 w i t h variable thickness : 234, 238, 326, 330, 360 simply s u p p o r t e d : 115, 134, 339, 439, 451, 530 strongly c l a m p e d : 503, 504, 525, 530, 548 thickness of a : 143 u p p e r face of a ~ : 148 weakly simply s u p p o r t e d u : 234 shell t h e o r y : C O S S B R A T - : 363, 549 DONNELL-MUSHTARI-VLASOV nonlinear s h a l l o w - : 555 first-order ~ : 550 f r a m e - i n d i f f e r e n t - : 452, 463, 466, 525, 541 geometrically exact m : 549 h i e r a r c h i c - : 368 higher-order i : 550 intrinsic linear u : 368 intrinsic n o n l i n e a r - : 551 large deformation, or large d i s p l a c e m e n t , - : 452, 463, 525 linear - - based on the m e t h o d of internal constraints : 368 linear BUDIANSKY-SANDERS ~ : 367 linear f l e x u r a l - : 101, 162, 171, 180, 182, 199, 526 linear K O I T E R ' S - : 100, 115, 336, 346, 548 linear m e m b r a n e u : 117, 126, 162, 170, 178, 182, 196, 199, 232, 246, 452, 466 linear NAGHDI'S u : 363, 365 linear s h a l l o w - : 369 MARGUERRE-VON KARMAN ~ : 552 multi-director ~ : 549 nonlinear B U D I A N S K Y - S A N D E R S : 551 nonlinear flexuzal ~ : 502, 505, 525 nonlinear K O I T E R ' S shallow ~ : 553 nonlinear K O I T E R ' S u : 547 nonlinear m e m b r a n e ~ : 439, 451, 463, 464, 505 nonlinear N A G H D F S ~ w i t h directors : 549 nonlinear shallow i : 552 nonlinear ~ b a s e d o n the m e t h o d of internal constraints : 550 NOVOZHILOV ~ : 371 one-director ~ : 363, 549

of higher-order : 550 of the first order : 550 time-dependent I. 234, 326, 347, 550, 551

simple s u p p o r t : t w o - d i m e n s i o n a l b o u n d a r y conditions of m : 115, 134, 339, 439, 451, 530 t w o - d i m e n s i o n a l b o u n d a r y conditions of weak - - : 234

Indez

596 s i n g u l a r p e r t u r b a t i o n p r o b l e m : 154 SOBOLEV spaces : 41

soft elastic m a t e r i a l : 464 s p h e r e : 67, 133, 135, 190, 441 s p h e r i c a l c o o r d i n a t e s : 15, 67 ST VENANT-KIRCHHOFF m a t e r i a l : 389, 392, 430 s t o r e d e n e r g y f u n c t i o n of a m : 391, 455, 459, 464, 467 s t a t i o n a r y p o i n t of a f u n c t i o n a l : 391, 448, 520, 523 s t e r e o g r a p h i c c o o r d i n a t e s : 67 s t o r e d e n e r g y f u n c t i o n : 391, 392, 4 5 1 , 4 5 5 , 4 6 3 strain : l i n e a r i z e d - s in CARTESIAN c o o r d i n a t e s : 9 linearized m s in curvilinear c o o r d i n a t e s : 36 scaled l i n e a r i z e d - : 153 scaled: 410 S i n CARTESIAN c o o r d i n a t e s : 388 s in curvilinear c o o r d i n a t e s : 398 s t r a i n e n e r g y : See " t w o - d i m e n s i o n a l s t r a i n e n e r g y " strain tensor : CAUCHY-GREEN-

: 9

linearized-

in CARTESIAN c o o r d i n a t e s : 9 G R E E N - S T V E N A N T - in CARTESIAN c o o r d i n a t e s : 388 G R E E N - S T VENANT - - i n c u r v i l i n e a r c o o r d i n a t e s : 397

stress : convergence o f - - e s : 234, 237, 326, 331 limites : 234, 237, 326, 331, 452, 546 l i n e a r i z e d - es in CARTESIAN c o o r d i n a t e s : 11 l i n e a r i z e d - es in curvilinear c o o r d i n a t e s : 38, 237 es in CARTESIAN c o o r d i n a t e s : 388 - - e s in curvilinear c o o r d i n a t e s : 402 stress couple : 344, 345 stress r e s u l t a n t : 224, 229, 344, 345, 450 stress t e n s o r : first P I O L A - K I R C H H O F F - : 388 l i n e a r i z e d - : 38 second P I O L A - K I R C H H O F F - : 387, 402 s t r o n g l y elliptic s y s t e m : 236 s u p p l e m e n t a r y c o n d i t i o n on L : 123, 236, 373 s u r f a c e : 65 d e v e l o p a b l e - : 83 elliptic ~ : 120, 293 hyperbolic: 295 infinitesimal rigidity of a ~ : 297 isometrics : 439, 441, 531 p a r a b o l i c - - : 296 rigidification of a - - : 297 r i g i d i t y of a - - : 442 surface force : See " a p p l i e d surface force"

597

Indez tensor : BUDIANSKY-SANDERS l i n e a r i z e d c h a n g e of c u r v a t u r e CAUCHY-GREEN s t r a i n (right) : 9 c h a n g e of c u r v a t u r e - - : 508 c h a n g e of m e t r i c m : 388, 398 c h a n g e o f m e t r i c - - o n a s u r f a c e : 437 curvature: 81 first PIOLA-KIRCHHOFF s t r e s s : 388, 403 G R E E N - S T VENANT s t r a i n : 388 linearized change of curvature: 93 linearized change of metric: 9, 36 l i n e a r i z e d c h a n g e o f m e t r i c - - o n a s u r f a c e : 91 l i n e a r i z e d s t r a i n ~ : 9, 36 l i n e a r i z e d s t r e s s ~ : 38 linearized transverse shear strain: 366 m e t r i c ~ : 18 m e t r i c ~ o n a s u r f a c e : 69 RIEMANN c u r v a t u r e : 136 s e c o n d PIOLA-KIRCHHOFF s t r e s s ~ : 387, 402 three-dimensional elasticity: 11, 32, 392, 396 t h r e e - d i m e n s i o n a l e l a s t i c i t y ~ of a shell : 148 t w o - d i m e n s i o n a l e l a s t i c i t y - - of a shell : 101, 117 Theorema

e g r e g i u m : 131, 136

thickness: shell with variable o f a shell : 143 three-dimensional

~ e

~

:

234, 238, 326, 330, 360

EUCLIDEAN s p a c e : 5

three-dimensional elasticity tensor : s c a l e d ~ : 154, 410 i n CARTESIAN c o o r d i n a t e s : 11, 59, 392 in c u r v i l i n e a r c o o r d i n a t e s : 32, 50, 59, 182, 396 three-dimensional energy : minimizer of a: 392 i n CARTESIAN c o o r d i n a t e s : 391 i n c u r v i l i n e a r c o o r d i n a t e s : 396 t h r e e - d i m e n s i o n a l e q u a t i o n s for a l i n e a r l y e l a s t i c shell : 146 s c a l e d ~ : 154, 200, 247, 307 three-dimensional scaled ~:

e q u a t i o n s for a n o n l i n e a r l y e l a s t i c shell : 406 410

three-dimensional EUCLIDEAN s p a c e : 5 three-dimensional linearized elasticity : in CARTESIAN c o o r d i n a t e s : 8 in c u r v i l i n e a r c o o r d i n a t e s : 32 three-dimensional nonlinear elasticity: i n CARTESIAN c o o r d i n a t e s : 391 i n c u r v i l i n e a r c o o r d i n a t e s : 401 time-dependent equations : for a l i n e a r l y e l a s t i c s h e l l : 234, 326, 347 for a n o n l i n e a r l y e l a s t i c shell : 550, 551 t o r u s : 66, 133, 292 t o t a l c u r v a t u r e : 82

: 367

598

Indez

transverse variable : 145, 150 average with respect to t h e - : 201 two-dimensional boundary conditions : u of clamping: 101, 116, 304, 305, 306, 322, 344 m of simple support : 115, 134, 439, 451, 530 m of strong clamping : 503, 504, 524, 525, 530, 548 of weak simple support : 234 two-dimensional constitutive equation : 229, 451 two-dimensional elasticity tensor of a shell : 101, 117, 190, 228, 291, 322, 338, 344, 365, 450, 524 s c a l e d - : 158, 170, 181, 210, 308, 430, 519 two-dimensional energy : of a linearly elastic elliptic membrane shell : 229 of a linearly elastic flexural shell : 322 of a linearly elastic generalized membrane shell : 290 of a nonlinearly elastic flexural shell : 524, 530 of a nonlinearly elastic membrane shell (theory derived by formal analysis) : 450 of a nonlinearly elastic membrane shell (theory derived by F-convergence): 463 two-dimensional equations" for a linearly elastic elliptic membrane shell : 117, 126, 210, 223, 227 for a linearly elastic flexural shell : 101, 309, 318, 320, 321 for a linearly elastic generalized membrane shell : 268, 283 for a nonlinearly elastic flexural shell : 518, 530 for a nonlinearly elastic membrane shell (theory derived by formal analysis): 444, 450 for a nonlinearly elastic membrane shell (theory derived by r-convergence): 463 two-dimensional equations of equilibrium : 229, 451 two-dimensional KOIT]~R energy : of a linearly elastic shell : 344 of a nonlinearly elastic shell : 548 two-dimensional KOITER equations : eigenvalue problem for the --- : 358 time-dependent m : 347, 361 for a linearly elastic shell : 100, 111, 115, 337, 339, 341, 344, 360, 373, 375 for a nonlinearly elastic shell : 547 two-dimensional KOITER strain energy : o f a linearly elastic shell : 344 o f a nonlinearly elastic shell : 548 two-dimensional strain energy (see also "two-dimensional KOITER strain energy") : o f a linearly elastic elliptic membrane shell : 229, 344, 361 of a linearly elastic flexural shell : 322, 344, 361 of a linearly elastic generalized membrane shell : 290 of a nonlinearly elastic flexural shell : 524, 548 of a nonlinearly elastic membrane shell (theory derived by formal analysis) : 450, 548 of a nonlinearly elastic membrane shell (theory derived by r-convergence) : 463

Indez

umbilical point : 82, 133 uniformly elliptic system : 123, 236, 237 uniqueness of solutions : 52, 101, 111,115, 122, 124, 126, 223, 317, 338, 340, 366, 367, 376, 530 upper face of a shell : 148 volume element : 18 weak lower semi-continuity of a functional : 431, 452, 536 WEINGARTEN (formula of--) : 88 Y O U N G modulus : 389

599