Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 www.elsevier.com/locate/cma On the theory of fourth-order tensors and their applications in computational mechanics Mikhail Itskov * Institut fur Statik und Dynamik, Ruhr-Universit at Bochum, Universit atsstraûe 150, 44780 Bochum, Germany Received 1 December 1998; received in revised form 29 November 1999 Dedicated to Professor Dr. -Ing. Yavuz Bas ar on the occasion of his 65th anniversary ß Abstract Many problems concerned with the mathematical treatment of fourth-order tensors still remain open in the literature. In the present paper they will be considered in the framework of a complete theory involving a set of notations and de®nitions, a tensor operation algebra, dierentiation rules, eigenvalue problems, applications of fourth-order tensors to isotropic tensor functions and some other relevant aspects. A tensor is understood to be an invariant quantity with respect to any co-ordinate system transformation, which justi®es the use of absolute notation preferred in this work. As a most important application ®eld of fourth-order tensors, elastic moduli are formulated in a material and a spatial description and given for various hyperelastic material models. Ó 2000 Elsevier Science S.A. All rights reserved. Keywords: Fourth-order tensors; Tensor algebra; Eigenvalue problems; Isotropic tensor functions; Tangent moduli 1. Introduction Fourth-order tensors as a mathematical object have found in the last 20 years a wide use in computational mechanics and especially in the ®nite element method. Their well-known applications are tangent (elastic or elasto-plastic) moduli as well as damage tensors playing an important role in the formulation of constitutive and evolution equations. The use of fourth-order tensors remains, nevertheless, extremely complicated because of the absence of a closed theory embracing many relevant aspects. In spite of active eorts in recent times (see [3±9,11,21,22,24,27±30,37,38,41,42]), there are many problems concerned with the treatment of fourth-order tensors, which are not completely solved and still remain open in the literature. · How can a fourth-order tensor be constructed from two second-order ones? · How can algebraic operations with fourth-order tensors be given in the absolute notation? · What does the derivative of a second-order with respect to another one mean? There is no uni®ed definition for the derivative with respect to a tensor. Is there a dierence in the de®nition of the derivative with respect to a symmetric second-order tensor? · How can the eigenvalue problem be formulated for fourth-order tensors and how can principal invariants and eigenvalues of a fourth-order tensor be calculated? How many irreducible invariants does a fourth-order possess? * Present address: Department of Applied Mechanics and Fluid Dynamics, University of Bayreuth, D-95440 Bayreuth, Germany. E-mail address: [email protected] (M. Itskov). 0045-7825/00/$ - see front matter Ó 2000 Elsevier Science S.A. All rights reserved. PII: S 0 0 4 5 - 7 8 2 5 ( 9 9 ) 0 0 4 7 2 - 7 420 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 The goal of the present paper is to try to solve these problems in a framework of the complete theory and to demonstrate then its application for the derivation of tangent moduli. The important characteristic feature of the development is the absolute notation used for tensor quantities throughout the paper. This is not only a notation manner but the basic concept of the paper. A tensor is understood to be an invariant quantity with respect to any co-ordinate system transformation and can be neither covariant, nor contravariant, nor mixedvariant in contrast to its components. In this connection, for example, the widespread use of the metric tensor as an argument of a function or as a dierentiation parameter seems to be meaningless, since the metric tensor represents in the end the identity tensor. Such notations always have to be accompanied by an indication of the component variance to be used in the present operation and will be avoided here. As a further crucial point of the paper it should be noted that in contrast to many other works we deal with arbitrary non-symmetric fourth-order tensors and understand them as a linear mapping of one arbitrary second-order tensor into another one (see also [19,29]). This considerably simpli®es the treatment of fourth-order tensors, which can be seen especially clearly in consideration of the eigenvalue problem. The symmetry properties of fourth-order tensors, which are relevant, for instance, for tangent moduli, can be enforced without loss of generality at the last stage of derivation. The starting point of the development is the set of notations and de®nitions given in Section 2. To have more freedom in construction of fourth-order tensors we propose a new tensor product of two second-order ones. The crucial point of the presented theory lies in a new de®nition of the derivative of one second-order tensor with respect to another one 2;2 . Due to this de®nition, the well-known product derivative rule valid for scalar values is proved to hold also for second-order tensors. The double contraction of a fourth-order tensor with a second-order one (4:2) is also rede®ned to be consistent with the dierentiation rule intro_ duced, such that the important rate relation A B A;B : B_ is satis®ed. Further, it is shown that the derivative with respect to a symmetric tensor is not unique and requires a slight correction in the de®nition. Special attention is paid in Section 2 to the transposition operations for fourth-order tensors and the resultant de®nition of a symmetric and a super-symmetric tensor. In this context, we introduce a special transposition operation bringing a fourth-order tensor to the standard de®nition of the tensor derivative. In the following this will permit to verify some important results by comparing them with those available in the literature. The indispensable part of the proposed theory is the algebra of fourth-order tensors given in Section 3. Simple, double, quadruple contractions and other operations with fourth-order tensors constructed from second-order ones are presented in absolute notation and can easily be proved using the de®nitions of the previous section. The following important topic is the formulation and proof of the dierentiation rules such as the product derivative and the chain rule. On this basis, we then obtain the derivative of the power tensor function for positive as well as negative integer exponents. Section 4 is devoted to the formulation of eigenvalue problems and spectral decomposition of fourthorder tensors. Using matrix representation the eigenvalue problem of a fourth-order tensor is reduced to that of a matrix and can then be solved by a standard procedure. For a symmetric fourth-order tensor this yields nine real eigenvalues and nine corresponding eigentensors. A complete analogy with the eigenvalue problem of a second-order tensor can be observed. On the basis of the other possible de®nitions for the double contraction 4:2 at whole 27 principal invariants and 27 eigenvalues of the fourth-order tensor can be received in this way. The discussed procedure is illustrated by spectral decompositions for a number of important fourth-order tensors like the identity, the trace projection and the transposition projection tensor. Application of the proposed theory to isotropic tensor functions is the topic of Section 5. Attention is focused on the representation of the derivative of an isotropic tensor-valued tensor function with respect to its argument, which is of major importance for the formulation and numerical calculation of tangent moduli in large strain elasticity and elasto-plasticity. We start with the consideration of a special class of isotropic tensor functions, which can be expanded in tensor power series. In the case of a symmetric tensor argument we receive for the derivative in question two closed-form representations. The ®rst one is expressed in terms of eigenvectors of the tensor argument and corresponds to the well-known result (see [9,27]). The second representation is given through the eigenvalue bases and is advantageous, as it avoids the numerically expensive computation of eigenvectors. In contrast to the analogous result by Miehe [24], M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 421 this representation does not use the derivatives of the eigenvalue bases and is obtained in a simpler and more compact form. The tensor algebra and dierentiation rules developed are applied in Section 6 to formulate tangent moduli in a material and a spatial description. It is proved that the tangent moduli presented are symmetric fourth-order tensors and permit consequently the spectral decomposition. The important question to be treated then is how the isotropy can be identi®ed by an elastic modulus. Using the spectral decomposition we prove that the elastic modulus corresponds to an isotropic material in the natural state if only it can be represented in the form of the St.Venant±Kirchho model involving two material parameters (see also [14,15,17,19,20,29,31] and references therein). Elastic moduli for this and some other hyperelastic material models such as Mooney±Rivlin and Ogden are given in Section 7. 2. Basic notations and de®nitions A second-order tensor (a bold capital letter): A Aij gi gj Aij gi gj Aij gi gj 2:1 A fourth-order tensor (a bold italics capital letter): k gi gj gk gl D Dijkl gi gj gk gl Dijkl gi gj gk gl Dijl 2:2 The simple contraction of arbitrary order tensors: m g i gl gm gn : AD Aij gi gj Dklnm gk gl gm gn Aij Djln 2:3 Tensor products of two second-order tensors are de®ned as follows: D A B Aij gi gj Bkl gk gl Aij Bkl gi gj gk gl ; 2:4 D A B Aij gi gj Bkl gk gl Aij Bkl gi gk gl gj : 2:5 It can easily be con®rmed the tensor products satisfy the distributive rule: A B C A B A C; A B C A B A C: 2:6 Transposition operations T and t for fourth-order tensors: T k k j gi gj gk gl Dijl g gi gl gk ; DT Dijl 2:7 k k gi gj gk gl t Dijl gi gk gj gl : Dt Dijl 2:8 T t Remark. One can easily prove that the transposition operations and are not commutative with each other: DTt 6 DtT . According to the above de®nitions the transposition applied to the tensor products (2.4) and (2.5) yields: T A B AT BT ; T A B B A; t A B A BT : 2:9 A symmetric fourth-order tensor (cf. [19,29]) DT D: 2:10 A super-symmetric fourth-order tensor ET E and E t E: 2:11 422 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 By means of the operation 0 1 E 0 E E t ; 2 2:12 a symmetric fourth-order tensor can be transformed into a super-symmetric one. Remark. For a fourth-order tensor some other transposition operations can be de®ned and particularly: k k gi gj gk gl R Dijl g i gl g j gk ; R : DR Dijl 2:13 which possess the important property A BR A B: 2:14 Double contractions of a fourth-order tensor with a second-order one 4 : 2 and 2 : 4 are de®ned by k k gi gj gk gl : Amn gm gn Dijl Ajk gi gl ; D : A Dijl 2:15 k k j gi gj gk gl Ail Dijl g gk : A : D Amn gm gn : Dijl 2:16 The double contraction of a fourth-order tensor with another fourth-order one (4:4): k n s ik jr n l gi gj gk gl : Amr D : A Dijl ns gm g gr g Djl Ank gi g gr g : 2:17 Evidently, the double contraction of fourth-order tensors is not commutative D : A 6 A : D, but can easily be proved to ful®l the associative rule: A : B : C A : B : C: 2:18 In contrast to the double contraction the scalar product (quadruple contraction) of two fourth-order tensors 4 :: 4 k k jl gi gj gk gl :: Amnsr gm gn gr gs Dijl Aik D :: A Dijl 2:19 obey the commutative rule: D :: A A :: D: 2:20 According to the de®nitions (2.15)±(2.17) and (2.19) the operations 2 : 4, 4 : 2, 4 : 4 and 4 :: 4 satisfy the distributive rule e.g.: A : B C A : B A : C; A B : C A : C B : C; 2:21 A : B C A : B A : C; A B : C A : C B : C; 2:22 A :: B C A :: B A :: C; A B :: C A :: C B :: C: 2:23 The second-order identity tensor: I g i gi : 2:24 The fourth-order identity tensor: I I I gi gi gj gj : 2:25 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 423 The trace of a fourth-order tensor is de®ned by tr D D :: I I :: D Diijj : 2:26 Powers of fourth-order tensors: D0 I; D1 D; D2 D : D; . . . Dn D : D{z : D | } : 2:27 n An inverse fourth-order tensor: D : Dÿ1 Dÿ1 : D I: 2:28 The matrix representation of a fourth-order tensor is de®ned through its mixedvariant components by 2 11 2 3 1 2 3 1 2 3 3 D11 D111 D111 D121 D121 D121 D131 D131 D131 1 2 3 1 2 3 1 2 3 7 6 D112 D112 D112 D122 D122 D122 D132 D132 D132 7 6 6 D1 1 D1 2 D1 3 D1 1 D1 2 D1 3 D1 1 D1 2 D1 3 7 6 13 13 13 23 23 23 33 33 33 7 6 21 2 3 1 2 3 1 2 3 7 7 6 D11 D211 D211 D221 D221 D221 D231 D231 D231 7 6 21 22 23 21 22 23 21 22 23 7 6 2:29 D 6 D12 D12 D12 D22 D22 D22 D32 D32 D32 7: 6 D2 1 D2 2 D2 3 D2 1 D2 2 D2 3 D2 1 D2 2 D2 3 7 6 13 13 13 23 23 23 33 33 33 7 6 31 2 3 1 2 3 1 2 3 7 7 6 D11 D311 D311 D321 D321 D321 D331 D331 D331 7 6 4 D3 1 D3 2 D3 3 D3 1 D3 2 D3 3 D3 1 D3 2 D3 3 5 12 1 D313 12 2 D313 12 3 D313 22 1 D323 22 2 D323 22 3 D323 32 1 D333 32 2 D333 32 3 D333 The partial derivative of a scalar-valued tensor function a A with respect to its second-order argument A 0;2 is given by a A;A oa oa i g gj o Aij gi gj oAij 2:30 and possesses the following important properties: 1. The derivative is independent of the choice of the component variance used in the dierentiation. Since Akl Akm gml , we have oa i oa oAkl i oa jl i oa i g g g gj g g gj g gl : j oAij oAkl oAij oAil oAil Similarly it can easily be proved also for the covariant components. 2. The derivative is independent of the choice of the co-ordinate system. In a transformed co-ordinate system we obtain: k k A Aij gi gj Al gk gl ) Al gk gi Aij gj gl ; k oa i oa oAl i oa k oa k g gj g gi gj gl gi gj g gl : i g gj k k k oA oAij oAl oAl oAl j These properties ensure the objectivity of the tensor derivative and justify the use of the absolute notation a A;A . Remark 1. Properties 1 and 2 and their proofs are not valid for the derivative with respect to the metric tensor. As mentioned above, the derivative with respect to the metric tensor is not objective since it depends not only on the component variance but also on the co-ordinate system used in dierentiation (see [16]). Remark 2. It is important to note that in the dierentiation with respect to a tensor its vector base is kept constant. Disregard of this fact may lead to an incorrect result. As a typical example we consider derivatives with respect to the Green±Lagrange and Almansi strain tensors 424 and M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 1 1 E C ÿ G gij ÿ Gij Gi Gj Eij Gi Gj 2 2 1 1 e g ÿ bÿ1 gij ÿ Gij gi gj eij gi gj ; 2 2 respectively, which are often used for the formulation of constitutive relations. It can be seen that these tensors have equal covariant components Eij eij related, nevertheless, to the dierent bases remaining constant in the dierentiation. Thus ! ! ow ow T ow ow ow ow T F F Gi Gj F F 2 Gi Gj FT 2 gi gj 6 g gj F oE oEij ogij ogij oe oeij i ÿ2 ow ow g gj ÿ2 g gj ; ÿ1 i oGij i obij which evidently contradicts the constitutive equation for the Cauchy stress tensor of the form s w;e (see e.g. [32]). The partial derivative of a second-order tensor C Cij Gi Gj with respect to another second-order one A Akl gk gl (2;2 ) is de®ned by C;A o Cij Gi Gj o Akl gk gl oCij oAkl G i gk gl G j 2:31 for the tensor bases Gi Gj of C, which are independent of the tensor components Akl . In other respect the choice of co-ordinate systems and the variance of components of both tensors A and C are irrelevant, which can easily be proved similarly to the properties of the derivative 0;2 . This ensures the objectivity of the de®nition (2.31) and justi®es the use of absolute notation for the tensor C;A . Remark. The derivative obtained according to the de®nition (2.31) can be transformed to the standard one R by means of transposition . Using (2.13) we have: R C;A oCij oAkl Gi Gj gk gl : The de®nitions (2.30) and (2.31) become non-unique if the tensor A is symmetric. In this case the dierentiation cannot still be carried out with respect to nine components of A, since only six of them are independent. This de®ciency can be eliminated by modifying the de®nitions (2.30) and (2.31). Accordingly the derivatives with respect to the symmetric tensor A AT can be de®ned by a A;A C;A 3 3 1X oa 1X oa i gi gj gj gi g gj gj gi 2 i;j 6 i oAij 2 i;j 6 i oAij 3 1X oa i g gj gj gi ; 2 i;j 6 i oAij 2:32 3 3 oCij oCij 1 X 1 X Gi gk gl gl gk Gj Gi gk gl gl gk Gj 2 k;l 6 k oAkl 2 k;l 6 k oAkl 3 oCij 1 X Gi gk gl gl gk Gj : 2 k;l 6 k oAkl 2:33 As can be observed the dierentiation in (2.32) and (2.33) is accomplished with respect to the six independent components of A and the resulting tensor is then symmetrized. M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 425 3. The algebra of fourth-order tensors In the following we summarize some important tensor identities, which will be intensively used in further derivation: T A B : C ACB; A B : C B : CA; C : A B AT CBT A B : C; C : A B C : AB; 3:1 3:2 A BC A BC; A BC AC B; C A B CA B; C A B CA B; 3:3 3:4 A B : C D AC DB; A B : C D B : CA D; T A B : C D ACB D; T T A B :: C D A : C B : D ; A B :: C D ACB : D; ÿ ÿ t A Bt : C D ADT CT B ; T T E : F F : E ; T t 3:6 A B :: C D A : D C : B; 3:7 T T E : A A : E; T A B :: C D A : C BD ; t T A B : C D AC B D; t 3:8 3:9 E : F E : F ; 3:10 T C : E C : E ; 3:11 A E : CB AEB : C: 3:12 t E :CE:C ; 3:5 A B : C D A C BD ; t T T The above relations directly emanate from the corresponding de®nitions (2.3)±(2.5), (2.7)±(2.8), (2.15)± (2.17) and (2.19). For example the identity 3:51 can easily be proved using (2.17), which leads to A B : C D Aij Bkl gi gj gk gl : Cmn Drs gm gn gr gs Aij Bkl Cjn Drk gi gn gr gl AC DB: By virtue of (2.31) we construct the partial derivative of a second-order tensor with respect to itself yielding the fourth-order identity tensor: A;A oAij oAkl gi gk gl gj dik dlj gi gk gl gj gi gi gj gj I: 3:13 The properties of the fourth-order identity tensor I following from (2.25), (3.1) and 3:51 can now be given by I : B B : I B; I : D D : I D: 3:14 Using (2.26), (3.7) and (3.8) the validity of the following important identities with the trace of a fourthorder tensor can also be proved: j kl Cij ; trC : D trD : C C : D :: I C :: D D :: C Dikl 3:15 trA B A B :: I tr Atr B; trA B A B :: I A : B; tr I I :: I I : I I : I 9; tr I I I I :: I I : I 3: 3:16 3:17 Due to the important property I I : A A : I I tr AI 3:18 the tensor I I introduced in 3:172 is referred to as the trace projection tensor. Remark. For the standard de®nition of the tensor derivative the trace projection tensor has the form ÿ R I IR gi gj gj gi gi gi gj gj I I: 426 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 Now, we construct the partial derivative of a second-order tensor with respect to its transverse counterpart delivering the transposition projection tensor T: A;TA A;AT oAij oAkl gj gk gl gi dik dlj gj gk gl gi I t T; 3:19 which possesses the following properties: T : B gj gi gj gi : Bkl gk gl Bij gj gi BT ; B : T BT : 3:20 For the derivative with respect to the symmetric part symA 1=2 A AT of a tensor A one receives under consideration of (2.12) and (2.33) 1 A;symA A;TsymA symA;symA I T I 0 : 2 3:21 Generalizing this result to the derivative of an arbitrary tensor delivers: B;symA B;A : A;symA B;A : I 0 B;A 0 : 3:22 Now, attention is focused on the tensor dierentiation rules. We start with the product derivative AB;C A;C B AB;C ; 3:23 which is well known for scalar values. According to the new de®nition of the derivative 2;2 (2.31) the product derivative rule (3.23) also holds for second-order tensors. Proof. AB;C o Aij Bjk gi gk o Clm gl gm oAij oClm o Aij Bjk oClm gi gl gm gk Bjk gi gl gm gk Aij oBjk gi gl gm gk A;C B AB;C : oClm Using this remarkable relation one can easily obtain the derivative of the tensor power function with respect to its argument B;nB n 1; 2 . . .. Considering (3.3), 3:51 and (3.15) one gets: B;2B B I I B; B;3B 3:24 2 2 2 nÿ1 X nÿ1 X nÿ1ÿr r Bnÿ1ÿr Br B I : I B ; 2 B I B B I B B I B I : I B I B ; B;nB r0 B;nB : I nBnÿ1 ; 3:25 3:26 r0 3:27 where we adopt B0 I. To obtain the derivative of the inverse function Bÿ1 ;B we ®rst use the identity: BBÿ1 ;B I;B 0, which leads by virtue of (3.3) and (3.23) to Bÿ1 ;B ÿBÿ1 Bÿ1 : 3:28 By analogue and exploiting (3.28) we can further write for the derivative of the power function with a negative integer exponent: M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 Bÿn ;B ÿ nÿ1 X Bÿrÿ1 Brÿn ; 427 3:29 r0 Bÿn ;B : I ÿnBÿnÿ1 : 3:30 Two other important dierentiation rules can be formulated as follows: aA;B A a;B aA;B ; A : B;C A : B;C B : A;C ; 3:31 where a denotes a scalar function. Proof. aA;B o aAij gi gj o Bkl gk gl o aAij oBkl oAij oa i k j gi g gl g k Aj gi g gl g a k gi gk gl gj oBl oBl k j A a;B aA;B ; A : B;C o Aij Bij o Ckl gk gl oAij oB j Aij ik Bij k oCl oCl ! gk gl A : B;C B : A;C : For the derivative of a scalar f A and a tensor-valued A C tensor function one can prove the following chain rules: f A;B A;B i of oAj k g gl f ;A : A;B ; oAij oBkl 3:32 oAij oCkl m j m gi g gn g A;C : C;B : oCkl oBn 3:33 4. Spectral decomposition, eigenvalues and principal invariants of a fourth-order tensor The double contraction 4:2 (2.15) establishes the basis for the formulation of the eigenvalue problems D : M kM 4:1 for a fourth-order tensor and enables then to determine its nine eigenvalues and principal invariants. To this end, we transform (4.1) as follows D ÿ kI : M 0: 4:2 This equation has a non-trivial solution 11 2 D11 ÿ k D111 D1 1 2 D112 ÿk 12 detD ÿ kI ... . . . D3 1 D3 2 13 13 M 6 0 if the corresponding characteristic equation 3 ... D131 13 D32 0; ... . . . . . . D3 3 ÿ k 4:3 33 which can also be presented in the form: ÿk9 ID k8 ÿ IID k7 IIID k6 IXD 0; 4:4 is ful®lled. In this equation the coecients ID ; IID ; IIID ; . . . ; IXD denote the principal invariants of the tensor D. On the basis of Newton formula and in view of the identity A : B A B they can be expressed in terms of principal traces of D (see also [42]): 428 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 ID tr D k1 k2 k3 k9 ; i 1h 2 IID ÿ tr D2 ÿ tr D k1 k2 k1 k3 k8 k9 ; 2 1 3 1 IIID tr D3 ÿ tr D2 tr D tr D3 k1 k2 k3 k1 k2 k4 k7 k8 k9 ; 3 2 2 1 4 1 1 2 2 4 IVD ÿ tr D4 ÿ tr D3 tr D tr D2 trD ÿ tr D2 tr D 4 3 2 6 4:5 k 1 k 2 k 3 k 4 k1 k2 k 3 k 5 k6 k 7 k 8 k 9 ; .. . IXD det D k1 k2 . . . k9 : In such a way the eigenvalue problem of a fourth-order tensor is transformed into the eigenvalue problem of its matrix representation and can then be solved by a conventional procedure of the linear algebra. Remark. The double contraction 4:2 (2.15) used for the formulation of the eigenvalue problem (4.1) is only one of three possible ones. Each of them would lead to its own matrix representation, eigenvalue problem and, ®nally, to its nine principal invariants. Thus one can obtain the basis of a fourth-order tensor consisting of its 27 invariants. The question about the integrity and irreducibility of this basis requires a special consideration (see [5]). T If the tensor D is symmetric, which immediately leads to symmetry of its matrix representation D D in an orthogonal co-ordinate system, the solution of the eigenvalue problems (4.1) yields nine real eigenvalues kn with the corresponding orthogonal eigentensors Mn n 1; 2; . . . ; 9. In this case the spectral decomposition of D is given by (the spectral theorem): D 9 X kr M r M r ; Ms : Mt dst : 4:6 r1 If the eigenvalues kn n 1; 2; . . . ; 9 of D are known and do not coincide, its eigenvalue bases Mr Mr can be presented by the closed formula [29,41]: M r Mr 9 Y D ÿ ks I s6r with kr ÿ ks n Y Ai A1 : A2 : An : 4:7 i If the tensor D is super-symmetric, which is relevant for the tangent moduli, its matrix representation in an orthogonal co-ordinate system includes three pairs of equal rows and columns and has the reduced rank 6. This means that at least three invariants and three eigenvalues of D are identically equal to zero. For the six eigentensors of D associated with non-vanishing eigenvalues one can obtain by virtue of 2:93 and 3:102 : t Mr Mr Mr MTr Mr Mr ) Mr MTr : 4:8 Thus, the spectral decomposition of a super-symmetric fourth-order tensor can be expressed in terms of only six eigenvalues and corresponding symmetric eigentensors (see also [11,12,21,30,35]): D 6 X kr M r M r ; r1 Mr MTr : 4:9 The closed formula solution for the eigenvalue bases (4.8) takes in this case the form: M r Mr 6 Y D ÿ ks I 0 : kr ÿ ks s6r 4:10 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 429 Concluding this section we present for example spectral decompositions of some important fourth-order tensors I, I I, T and I 0 : I 3 X ÿ ÿ ni nj ni nj ; k1 k2 k9 1; 4:11 k1 3; 4:12 i;j1 1 1 I I 3 p I p I ; 3 3 T 3 X ni ni ni ni i ÿ k2 k3 k9 0; 3 X 1 ÿ 1 ÿ p ni nj nj ni p ni nj nj ni 2 2 i;j<i 3 X 1 ÿ 1 ÿ p ni nj ÿ nj ni p ni nj ÿ nj ni ; 2 2 i;j>i k1 k2 k6 1; k7 k8 k9 ÿ1; 4:13 3 3 X X 1 1 ÿ 1 ÿ p ni nj nj ni p ni nj nj ni ; ni ni ni ni I 0 I T 2 2 2 i i;j<i k1 k2 k6 1; 4:14 k7 k8 k9 0 with ni i 1; 2; 3 being a set of orthogonal unit vectors: ni nj dij . 5. Application to isotropic tensor functions A tensor-valued tensor function G A is said to be isotropic if it satis®es the relation [39]: G QAQT QG AQT 5:1 ÿT for an arbitrary orthogonal tensor Q Q . In the further derivation we shall ®rst deal with tensor power series building a special class of isotropic tensor functions: 2 3 G A g0 I g1 A ÿ aI g2 A ÿ aI g3 A ÿ aI ; 5:2 where gi and a are scalar-valued constants. These functions are referred here to as analytical tensor functions. For instance, isotropic tensor functions such as exponential and logarithmic ones being important and often used in computational mechanics are de®ned in the form (5.2) by exp A I A 1 2 A ; 2! 5:3 1 1 2 3 ln A A ÿ I ÿ A ÿ I A ÿ I 2 3 5:4 Our purpose is to obtain the derivative of an isotropic function with respect to its argument, which is of high importance in computational elasticity and elasto-plasticity for the construction of tangent moduli. Using the relation (3.26) and setting in (5.2) without loss of generality a 0, we receive for the derivative of an analytical tensor function G A;A g1 I g2 A I I A gn rnÿ1 X r0 Anÿ1ÿr Ar 5:5 430 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 On the basis of expression (5.5) the important identity for the time derivative can be con®rmed as follows _ gn G A;A : A_ g1 A_ g2 AA_ AA rnÿ1 X _ _ r G A: Anÿ1ÿr AA 5:6 r0 The representation (5.5) holds for arbitrary tensors. In the special case of a symmetric tensor argument A AT the derivative G A;A takes the form: G A;A g1 I 0 g2 A I I A0 gn rnÿ1 X Anÿ1ÿr Ar 0 5:7 r0 and can expressed by means of the spectral decomposition of A A k 1 n1 n1 k2 n2 n2 k3 n3 n3 ; by G A;A 1 X " gn n 3 X a n1 knÿ1 a na 5:8 na n a n a rnÿ1 X 3 X r0 a;b6a # knÿ1ÿr krb na a 0 na n b nb : 5:9 It can easily be seen that the derivative (5.9) presents a super-symmetric fourth-order tensor in the spirit of de®nition (2.11): T G A;A G A;A ; t G A;A G A;A : Introducing the abbreviation for the diagonal function [24] G k representation for G(A) P1 n0 5:10 gn kn allowing the alternative G A G k1 n1 n1 G k2 n2 n2 G k3 n3 n3 ; 5:11 the relation (5.9) can be given in the case of distinct eigenvalues ki in terms of eigenvectors ni by G A;A 3 X G0 ka na na na na 3 X G ka ÿ G kb 0 na na nb nb ÿ k k a b a;b6a G0 ka na na na na 3 1 X G ka ÿ G kb na na nb nb na nb : 2 a;b6a ka ÿ kb a 3 X a 5:12 Applying the operation R (2.13) to the relation (5.12) we can return G A;A to the standard de®nition of the tensor derivative: G A;A R 3 X G0 ka na na na na a 3 1 X G ka ÿ G kb na nb na nb nb na ; 2 a;b6a ka ÿ kb 5:13 which corresponds to the well known result [9,27]. In terms of the eigenvalue bases Mi ni ni i 1; 2; 3, which can be obtained by means of the closedformula solution [2,26,36], the derivative (5.13) is expressible in the form: G A;A 3 X a G0 ka Ma Ma 3 X G ka ÿ G kb 0 Ma Mb : k ÿ k a b a;b6a 5:14 The last representation has the advantage, that it avoids a numerically expensive determination of eigenvectors. Comparing with the analogous solution by Miehe [22,24] it is observable that the representation (5.14) does not include the derivatives of the eigenvalue bases and has a simpler and more compact form. The special cases of two or three equal eigenvalues ki require a special treatment. Considering in (5.14) the limit case ka ÿ kb D ! 0, one can obtain the following results: M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 431 1. Triple coalescence of eigenvalues: k1 k2 k3 k; A kI, G A;A G0 kI 0 : 5:15 2. Double coalescence of eigenvalues: ka 6 kb kc k; A ka Ma k I ÿ Ma , G ka ÿ G k 0 Ma I ÿ Ma I ÿ Ma Ma ka ÿ k 0 G0 k I ÿ Ma I ÿ Ma : G A;A G0 ka Ma Ma 5:16 According to the representation theorem [39] an arbitrary isotropic tensor function, which cannot generally be presented via power series (5.2), is given in the form: G A u0 AI u1 AA u2 AA2 ; 5:17 where ui A ui QAQT are scalar-valued isotropic tensor functions of A. By virtue of (3.13), (3.24) and (3.31) we construct the derivative G A;A by G A;A u1 AI u2 A A I I A I u0 A;A A u1 A;A A2 u2 A;A ; 5:18 where exploiting the isotropy of ui : ui A ui IA ; IIA ; IIIA their derivatives can be given by ui A;A oui oui oui T oui IA I ÿ A IIIA AÿT : oIA oIIA oIIA oIIIA 5:19 Using the result (5.18) and (5.19) and by virtue of (3.1) and (3.2) it can easily be proved that the relation: AG A;A : lA G A;A A : Al AG A;A : I A : l I A : G A;A : A I : l; 5:20 where l presents an arbitrary second-order tensor, holds for symmetric tensors A AT . For the time derivative of an arbitrary isotropic tensor function we obtain by using (3.1), (3.2), (3.14), (5.18) and (5.19) the well-known relation: _ _ Iu_ 0 A Au_ 1 A A2 u_ 2 A G A: G A;A : A_ u1 AA_ u2 A AA_ AA 5:21 To complete this section we give the derivatives of some isotropic tensor functions, which cannot be expanded in power series (5.2): tr AI;A I trA;A I I; 1 1 devA;A A ÿ trAI ;A I ÿ I I P 3 3 5:22 5:23 with P being the deviatoric projection tensor: A : P P : A devA. 6. Tangent moduli One of the most important applications fourth-order tensors ®nd in computational elasticity and elastoplasticity, where they appear as tangent or elastic moduli. The algebra operations and dierentiation rules presented above now enable to formulate tangent moduli in absolute notation and discuss then their properties. The formulation succeeds in spatial as well as material descriptions. Important notations to be exploited in this context are: 432 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 w w C F gi Gi C FT F b FFT E 12 C ÿ I S s FSFT C; c _ ÿ1 l FF d 1=2 l lT Lm a a_ ÿ la ÿ alT energy density function (per unit volume of the undeformed body), deformation gradient, right Cauchy-Green tensor, left Cauchy±Green tensor (Finger tensor), Green±Lagrange strain tensor, second Piola±Kirchho stress tensor, Kirchho stress tensor, tangent(elastic) moduli in material and spatial description respectively, spatial gradient of velocity, rate of deformation tensor, Lie derivative (Oldroyd rate) of a spatial tensor a aij gi gj . We start with the general de®nitions of the tangent moduli. Using the Doyle±Ericksen formula [13] and by virtue of relations (3.1) and 3:122 the tangent moduli are constructed such that they satisfy the corresponding constitutive rate equations. Material description: ow ow ; oC oE o2 w o2 w C4 oCoC oEoE oS 1 1 _ : C_ C : C_ C : E: S_ 2 oC 2 2 S2 6:1 6:2 6:3 Spatial description: s 2F ow T F ; oC 6:4 o2 w : FT F cabcd FaA FbB FcC FdD CABCD ; oCoC o2 w _ o2 w T T _ : E FT 4F F : FT dF c : d: Lm s FSF F 4 oCoC oCoC c F FT : 6:5 6:6 The expression of the tangent modulus in the spatial formulation (6.5) coincides with the well-known representation [33]: c2 os o2 w 4 ; og ogog 6:7 if only the derivation in (6.7) is carried out with respect to the covariant components of the metric tensor g gij gi gj in the current con®guration and it is assumed that the covariant vector bases of s sij gi gj are independent of gij . This leads to c os osij oS T o2 w F : FT F F FT : : FT F; gi gk gl gj F og ogkl oC oCoC 6:8 which is evidently identical with (6.5). Such a derivative of a tensor, where its basis is kept constant, is analogical to the Lee derivative. Otherwise, the dierentiation with respect to the metric tensor in the spirit of the de®nition (2.31) would lead to a meaningless result, since g presents the identity tensor. Material and spatial formulations presented are valid both for isotropic and anisotropic materials. In literature there exists also a spatial representation of the elastic modulus in term of the left Cauchy±Green tensor b proposed by Miehe [23] for isotropic materials c 4b o2 w b; obob Lm s c : d: 6:9 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 433 In the following we show, that the de®nition of the material tensor 6:91 leads to the rate relation 6:92 if only one assumes that the tensor b is not symmetric while derivating with respect to b. To prove this we ®rst transform the elastic modulus 6:91 to the proposed de®nition (2.31) of the tensor derivative. Then c 4 b I : o2 w o2 w : I b 4 I b : : b I; obob obob 6:10 such that o2 w c 4 b brl i k gm gk gr gj obj obl mi R !R 4bmi brl o2 w o2 w b: g gj gk gr 4b i k m obob obj obl Using the constitutive relation for isotropic materials in the form s 2w;b b 2bw;b and by virtue of (2.33), (5.20) and (3.11) one can obtain: h i i h 0 0 Lm s s;b : b_ ÿ ls ÿ slT 2I w;b 2bw;bb : lb 2w;b I 2w;bb b : blT ÿ ls ÿ slT 1 1 4 I b : w;bb : b I : d blT w;b w;b lb ÿ ls slT c : d blT w;b w;b lb ÿ ls slT : 2 2 On the contrary, assuming b is not symmetric in the dierentiation and using the corresponding de®nition of the tensor derivative (2.31) we receive: Lm s 2I w;b 2bw;bb : lb 2w;b I 2w;bb b : blT ÿ ls ÿ slT 4 I b : w;b : b I : d 2lT bw;b 2w;b bl ÿ ls slT c : d: It can easily be proved that the tangent moduli C (6.2) and c (6.5) are super-symmetric according to their de®nitions. For C it directly follows from (5.10). As to c we have by using (2.9), (3.9) and (3.10) 2 T T o2 w ow : FT F FT FT : : F FT T c; cT F FT : oCoC oCoC " #t t t o2 w o2 w T T T : F F F F : : F F c F F : oCoC oCoC 2 tt ow T T : F F c: F F : oCoC 6:11 T t 6:12 Similarly, the symmetry can also be proved for the other elastic modulus A o2 w ; oFoF A AT ; 6:13 which is used in literature, too [33]. The super-symmetry of the elastic moduli C (6.2) and c (6.5) permits their spectral decomposition in the form (4.9). For example we get for C C 6 X r1 kr M r M r ; Mr MTr : 6:14 Now, the question is what properties the elastic modulus corresponding to an isotropic material possesses and how the isotropy can be identi®ed by tangent moduli. This problem can easily be solved for the natural state, where b C I. In this case the tensor function dS dE C : dE should satisfy the isotropy condition: QdSQT C : QdEQT 6:15 434 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 for an arbitrary strain variation dE and an arbitrary orthogonal tensor Q QÿT . Using the decomposition of dE in terms of Mr : dE 6 X dEr Mr ! QdEQT r1 dS dEr QMr QT 6:16 r1 we obtain then from (6.14): 6 X 6 X ! kr M r Mr 6 X : r1 ! dEs Ms s1 6 X kr dEr Mr : 6:17 r1 Under consideration of (6.17) the condition (6.15) takes then the form: 6 X kr dEr QMr QT r1 6 X 6 X r1 kr dEs Mr : QMs QT Mr : 6:18 s1 Contracting the left- and right-hand sides with Mt yields 6 X 6 6 X X kr dEr Mt : QMr QT kt dEr Mt : QMr QT ! kt ÿ kr dEr Mt : QMr QT 0 r1 r1 8dEr and r1 ÿT 8Q Q : 6:19 Since eigentensors Mt are symmetric the condition (6.19) can be satis®ed only in two following cases: 1: k1 k2 k6 2l ! C 2lI 0 ; 1 2: k1 3k; M1 p I; k2 k6 0 ! C kI I; 3 6:20 6:21 where 2l and k denote material constants. Generally we can state that an elastic modulus corresponds to an isotropic material in the natural con®guration, if and only if C can be represented via linear combination of the tensors I 0 and I I in the form of the St. Venant±Kirchho model (see also [14,15,17,19,20,29,31]): C 2lI 0 kI I: 6:22 The analogous statement for the constitutive relations has been proved by Ciarlet [10]. 7. Examples of elasticity tensors Using the results (6.1), (6.2), (6.4) and (6.5) of the previous section as well as tensor algebra operations and dierentiation rules (3.5), (3.6), (3.9), (3.10), (3.13)±(3.15), (3.22), (3.23), (3.28), (3.31)±(3.33), (5.21) and (5.22), we derive here tangent tensors in material and spatial descriptions for a number of hyperelastic material models intensively used in continuum mechanics. 1. St.Venant±Kirchhoff material model: 1 2 2 w j tr E l tr devE ; 2 7:1 k and l being the compression and shear moduli respectively. Material description: 2 ow otr dev E o dev E j tr EI l : j tr EI 2l dev E; oE o dev E oE oS 1 jI I 2l I 0 ÿ I I : C oE 3 S 7:2 7:3 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 435 Spatial description: 1 s FSFT j tr b ÿ 3b lb dev b; 2 1 0 T T c F F : C : F F jb b 2l b b ÿ b b : 3 7:4 7:5 2. Mooney±Rivlin material model [25]: w C1 IC ÿ 3 C2 IIC ÿ 3 C1 Ib ÿ 3 C2 IIb ÿ 3; 7:6 where C1 and C2 are material constants. Material description: ow 2C1 I 2C2 IC I ÿ C; oC oS 4C2 I I ÿ I 0 : C2 oC S2 7:7 7:8 Spatial description: ow b 2C1 b 2C2 IC b ÿ b2 ; ob h i 0 c F FT : C : FT F 4C2 b b ÿ b b : s FSFT 3. Ogden material model [27]: X lr ÿ a k1r ka2r ka3r ÿ 3 ; w ki ar r 7:9 7:10 7:11 where ki denote the eigenvalues of the right stretch tensor U and ar ; lr are material parameters. Material description: S 2 aI aII IC I ÿ aII C aIII IIIC Cÿ1 ; h C 4 cII : 2cI II IC cII II I2C bII I I cII II C C IIIC bIII cIII III IIIC Cÿ1 Cÿ1 ÿ cI II cII II IC I C C I IIIC cI III cII III IC I Cÿ1 Cÿ1 I i 0 ÿ IIIC cII III C Cÿ1 Cÿ1 C ÿ bII I 0 ÿ IIIC bIII Cÿ1 Cÿ1 : Spatial description (cf. [18]): s 2 aI aII Ib b ÿ aII b2 aIII IIIb I ; h c 4 cII : 2cI II Ib cII II I2b bII b b cII II b2 b2 IIIb bIII cIII III IIIb I I ÿ cI II cII II Ib b b2 b2 b IIIb cI III cII III Ib b I I b i 0 ÿ IIIb cII III b2 I I b2 ÿ bII b b ÿ IIIb bIII I 0 : 7:12 7:13 7:14 7:15 Using the alternative representation form of the energy function w w IC ; IIC ; IIIC the unknown coecients appearing in (7.12)±(7.15) a K bK ow ; oK cKL o2 w ; oKoL K; L IC ; IIC ; IIIC 7:16 can be specialized for an arbitrary isotropic material model. For the Valanis±Landel hypothesis [40] and its special case Ogden model (7.11) these coecients have been determined by Bas ar and Itskov [1] for the ß problems. cases of distinct as well as equal eigenvalues without explicit solving the eigenvalue 436 M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 4. Material models with decoupled volumetric±isochoric response. For these models the energy function is assumed to be additively split into volumetric and isochoric parts: 7:17 w U J W C; where J IIIC 1=2 ; C J ÿ2=3 C: 7:18 Accordingly the corresponding stress tensors and elastic moduli permit the additive decomposition: S Svol Siso ; s svol siso ; C Cvol Ciso ; c cvol ciso 7:19 7:20 and take the following form: Material description: Svol 2 oU U 0 J Cÿ1 ; oC 7:21 Siso 2 ÿ oW oW oC S iso ; : 2 Siso : p dev Siso C Cÿ1 Cÿ1 dev C oC oC oC 7:22 ÿ 0 oSvol ÿ 00 2 U J U 0 J Cÿ1 Cÿ1 ÿ 2U 0 J Cÿ1 Cÿ1 ; oC 7:23 Cvol 2 0 ÿ oSiso oSiso ÿ 2Cÿ1 P0 : C I Siso : p ÿ 2 Cÿ1 Cÿ1 0 dev C Siso oC oC h 0 i ÿ 0 ÿ ÿ1 : p ÿ 2 Cÿ1 Siso ; pT : Ciso : 2 C : Siso Ciso 2 7:24 where Siso 2 oW ; oC Ciso 2 oSiso o2 W ; 4 2 oC oC 7:25 oC oJ ÿ2=3 1 J ÿ2=3 I 0 ÿ C Cÿ1 J ÿ2=3 I 0 : C p oC oC 3 Spatial description: svol FSvol FT U 0 J I; 7:26 T siso FSiso F devsiso ; 7:27 T T T T 00 2 0 0 0 cvol F F : Cvol : F F U J U J I I ÿ 2U J I ; 0 ciso F F : Ciso : F F P : ciso 2 I siso : P ÿ 2 I siso 2 2 P0 : ciso : P0 tr siso P0 ÿ siso I I siso ; 3 3 7:28 0 7:29 where T siso F Siso F ; T T ciso F F : Ciso : F F; F J ÿ1=3 F: R 7:30 It can easily be seen that after the transformation the expressions (7.23) and (7.24) coincide with those given by Simo and Taylor [34]. In the spatial description we have forgone to use the de®nition (6.9) M. Itskov / Comput. Methods Appl. Mech. Engrg. 189 (2000) 419±438 437 for the isochoric moduli ciso . For this reason the representation (7.26)±(7.29) holds in contrast to the analogous result by Miehe [23] not only for isotropic but also for anisotropic materials. 8. Conclusion In the paper we have presented a theory of fourth-order tensors. The theory enables to solve many relevant problems in the treatment and application of fourth-order tensors, which are still open in the literature. Starting with the set of notations and de®nitions we have presented in absolute notation the tensor algebra and dierentiation rules, which are applied then to isotropic tensor functions. The important result to be emphasised is a closed-formula solution for the derivative of an isotropic tensor function, which is given in terms of eigenvalue bases for the cases of distinct and equal eigenvalues. This solution has a simpler and more compact form in contrast to those known in the literature. The next important topic are the eigenvalue problems and the spectral decomposition of a fourth-order tensor. It is shown that the eigenvalue problem of a fourth-order tensor can be reduced to that one of its matrix representation and then easily solved. This leads to a spectral decomposition involving nine eigenvalues and nine corresponding eigentensors. In the case of super-symmetry characterizing for example some tangent moduli, the spectral decomposition can be given through only six symmetric eigentensors. Concerning the invariants of a fourth-order tensor we have come to their total number of 27, which can be obtained using various contraction rules with a second-order tensor. A most important application of the fourth-order tensors are tangent moduli. 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