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The Structure of the Elastic Tensor

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1 The Structure of the Elastic Tensor
A study of the possibilities opened up by Kelvin 150 years ago Klaus Helbig, Hannover The Structure of Tensors

2 The customary “official” representation
The tensor cijkl connects the symmetric stress tensor ij symmetrically with the symmetric strain tensor ekl The tensor cijkl has 34=81components The two “symmetries” of stress and strain mean  ij = ji , kl = lk , thus cijkl = cjikl = cijlk The “symmetrical” connection means cijkl = cklij Thus only 21 of the 81 components are significant! The Structure of Tensors

3 Hooke’s Law There are still 36 terms, but, e.g., c2313=c1323
The Structure of Tensors

4 The Voigt mapping 2E = ij ij = pp
With only 21 significant components, the elastic tensor can obviously be mapped on a symmetric 66 matrix Such “mapping” should preserve the elastic energy density 2E = ij ij = pp The Voigt mapping achieves this by the mapping rules p = i ij+ (1–ij)(9–i–j ) , q = k kl+ (1–kl)(9–k–l ) p = ij , cpq = cijkl , q = (2 – kl )kl The Structure of Tensors

5 The Voigt mapping, visual
11 12 13 22 23 33 11 22 33 23 13 12 11 12 13 22 23 33 11 22 33 23 13 12 11 22 33 23 13 12 Mapping for the stress tensor Mapping for the strain tensor But this would not keep the scalar product s.! But this does. The Structure of Tensors

6 Properties of the Voigt mapping
Advantages The Voigt mapping preserves the elastic energy density The Voigt mapping preserves the elastic stiffnesses Disadvantages Stress and strain are treated differently The norms of the three tensors are not preserved The entries in all three Voigt arrays are not tensor- or vector components, thus we loose all advantages of tensor algebra The Structure of Tensors

7 Lost Advantages of Tensor Algebra
There is no “invariant representation” Representation in another coordinate system by the simple rule ’kl = rki rlj ij is not possible For rotation of the coordinate system, one has to use the Bond relations, Mohr’s Circle, and other constructs. The Structure of Tensors

8 The Kelvin mapping 2E = ij ij = pp
The Kelvin mapping preserves E by the mapping rules p = i ij+(1-ij)(9–i–j ) , q = k kl+ (1–kl)(9–k–l ) p = (ij+√2(1–ij )) ij , q = (kl+√2(1–kl)) kl , Cpq = (ij+√2(1– ij )) (kl+√2(1– kl)) cijkl , The Structure of Tensors

9 Properties of the Kelvin mapping
Advantages The Kelvin mapping preserves the elastic energy density The norms of the three tensors are preserved Stress and strain are treated identically The “maps” of stress, strain, and stiffness have all properties of tensors of 1st respectively 2nd rank in 6D-space, thus we keep all advantages of tensor algebra Only disadvantage: the values of the stiffness components are changed The Structure of Tensors

10 A tensor is a tensor by any name!
It is important to realize that a tensor is a physical entity that does not depend on the way we describe it. For instance: if in a mapping (a change of description) the norm of the tensor is not defined (as in the Voigt mapping), it does not mean that the norm is lost, only that we cannot access it easily as long as we use this description. The description we choose is not a question of ideology, but of scientific economy: for many problems the Voigt mapping is the natural choice, but there are problems that are much more easily solved in the Kelvin form. For some problems the 4th-rank tensor is the most convenient notation. The Structure of Tensors

11 Which notation? Each has is place!
The Voigt notation is the de facto standard in the “outside world”: in the entire literature, elastic parameters are listed in this notation, and “users” expect that results are listed in this form. For this reason, algorithms to deal with tensors in Voigt notation are useful. The strength of the Kelvin notation is the possibility to reduce an elastic tensor to its invariant (coordinate free) representation, and conversely to “construct” tensors with given invariants. It should be used in the analysis of tensors. The 4-subscript tensor notation is convenient for operations as the change of coordinate systems: the very definition of a tensor is based on this operation. The Structure of Tensors

12 Practical aspects of multiple notations
Even ten years ago, a conversion from one notation to another was not a trivial matter, and the 6561 multiplications needed for a transformation of the coordinate system might have taken up to a minute. Today a scientist is hardly ever without access to a computer, and the relevant routines can be freely exchanged. Most of the important operations give results “instantly”, i.e., with response times below two seconds. The current project will be completed with a Tensor Toolbox written as a Mathematica notebook. In “Reader” format it can be used on any computer without the program. The Structure of Tensors

13 A simple tool for conversion
For conversion between the Voigt- and Kelvin notation, only one array is needed: = 1 √2 K = V  V = K/ K = V /  V = K  For the stiffnesses, one uses the “outer product” of  1 √2 2 CK = CV The Structure of Tensors

14 How did Kelvin come to his description?
Not as a mapping of a 4th-rank 3D tensor on a 2nd-rank 6D tensor, because neither did exist then. The line of thought can be described like this: 1. A strain can be described by 6 linearly independent “base strains”. 2. A stress can be described by 6 linearly independent “base stresses”. 3. It is convenient to use bases of the same “type” for stress and strain. 4. It is convenient to use a set “orthogonal types” for the common basis. 5. The “weight” of the different components should be such that the product of a“parallel” pair of stress and strain is preserved under coordinate transformations from one to another orthonormal base (hence the √2). In this way Kelvin had defined a 6D Cartesian vector space The Structure of Tensors

15 Kelvin went on to the invariant description
Hooke’s law can be thought of as a linear mapping of the strain space on the stress space The map is described by the 66 stiffness matrix 6. The ideal base strain generates a parallel base stress (of the same type). Kelvin called such strains “principle strains”, we call them “eigenstrains”. As examples he gave for isotropic media “hydrostatic pressure” -> “uniform volume compression” and “shear strain” -> “shear stress”. 7. In a base consisting of (orthogonal) eigenstrains, the 66 representation of the stiffness tensor is diagonal, with the “eigenstiffnesses” the only non-zero components. Kelvin thus had produced the “eigenvalue decomposition” – or the “canonical representation of the stiffness tensor by its invariants”. The Structure of Tensors

16 Eigensystem of isotropic media
The Structure of Tensors

17 The Structure of Tensors
Nomenclature I have called the eigenvalues eigenstiffnesses, and the eigenvectors eigenstrains. Why these special terms? A similar eigenvalue problem exists for the inverse of Hooke’s Law. The resulting items are called eigencompliances and eigenstresses. The nature of the 6 eigenstrains is of great importance for many tasks, but not easily seen in an arbitrarily oriented coordinate system. If these details are important, the eigenstrain vectors are treated as 33 tensors and brought into invariant (canonical) form. The elements of these representations are called eigenvalues and eigenvectors. The Structure of Tensors

18 How does eigenvalue decomposition work in the different notations?
The “eigenvalue decomposition” can be formulated as: find a stress that is generated by a parallel strain Four-subscripts: ij = cijkl kl=ij =>(cijkl – ikjl ) kl = 0 Meaningful problem, solution has to be programmed Kelvin notation: p = Cpq q = p => (cpq - pq) q= 0 Standard eigenvalue/eigenvector problem, routines for solution in every math-package Voigt notation: the problem cannot be formulated easily, since stresses and strains are expressed in terms of different bases. The Structure of Tensors

19 What does the invariant description mean?
Of the 21 parameters of a general elastic tensor, only the six eigenstiffnesses are genuinely elastic The remaining 15 parameters are geometric: the 15 free parameters that describe a set of six mutually perpendicular 6D unit vectors Of these 15, three are extraneous to the problem: they are the “Euler angles” that describe the orientation of the material with respect to the global coordinate system Conjecture: All geometric parameters must be real. Only the eigenstiffnesses can assume complex values. The Structure of Tensors

20 How does all this affect our work?
The “invariant description” is possible for every medium. Obviously the medium is stable if all six eigenstiffnesses are positive. In modeling a dissipative medium one cannot freely assign imaginary parts to the stiffnesses. If we would do that, we might end up with complex eigenstrains, in violation of the concept of a “strain type”. How do we assign imaginary parts to the 21 stiffnesses? We need a method to construct tensors from their eigensystem, i.e., a “eigenvalue composition”. The Structure of Tensors

21 Eigenvalue composition of a tensor
If E is a 66 orthonormal matrix and L is a diagonal matrix with 6 positive elements, then C = E .L.ET is a symmetric, positive definite, 66 matrix with the elements of L as eigenvalues and the column vectors of E as eigenvectors If we choose the intended eigenstrains as column vectors of E and place the intended eigenstiffnesses on the diagonal of L, we can generate a stiffness tensor C with an arbitrarily chosen eigensystem. The Structure of Tensors

22 How should the eigensystem be chosen?
Obviously, the symmetry of the stiffness tensor – and some other properties like the “order” of elastic waves – is controlled by the chosen eigensystem. An “educated” choice requires that we know more about the nature of the eigenstrains and the way they influence (together with the eigenstiffnesses) the stiffness tensor. Such a study is not necessary if we just want to make an existing tensor “dissipative”: we just have to determine the eigensystem, add imaginary parts (of the correct sign) to the eigenstiffnesses, and re-compose. The Structure of Tensors

23 Example: a dissipative orthotropic medium
The following complex-valued stiffness tensor C was used: i i i i i i i i i Kelvin form The real part was “invented” in 1991, the imaginary part came from a different source. Are these data consistent with our assumptions? The Structure of Tensors

24 The eigensystem of the tensor C
i i i i i i i .737 i .693 i i i i .93 1 All eigenstiffnesses have a small imaginary part, but so have two components of each of three eigenstrains. What does that mean? Moreover, this matrix is not orthonormal ! The Structure of Tensors

25 The improved dissipative tensor C’
The real part of the eigenstrains together with the complex eigenstiffnesses result in: Kelvin form i i i i i i i i i The changes are moderate, but now everything is consistent. Note: the shear stiffnesses have not changed at all. The “shear”eigenstiffnesses are equal to the corresponding shear stiffnesses (in Kelvin form) The Structure of Tensors

26 Anatomy of the strain tensor
Since the appearance of the eigenstrains depends on their orientation with respect to the global coordinate system (three Euler angles!), we have to look at the invariant representation of strains. Any (unit) strain tensor can be part of the eigensystem of a stable stiffness tensor Two invariants of a strain tensor are the trace and the determinant Strains with vanishing trace are called “isochoric” Strains with vanishing determinant are called “wave-compatible” The Structure of Tensors

27 The Structure of Tensors
Wave compatibility? The term “wave compatible” sounds oddly out of place in a discussion that so far concerned only static aspects. Consider a homogeneous strain in an unbounded medium. Even an infinitesimal strain can lead to very large displacements at large distance from the reference point. Homogeneous strain in unbounded media cannot exist. Some homogeneous strains can exist along a plane. The Structure of Tensors

28 “Wave compatibility” explained
Ultimately we are interested in plane waves. Any displacement can be attached to a plane wave, but only those strains that can exist along a plane without creating infinite displacements. Such strains are “compatible” with wave propagation perpendicular to the plane. Hence their name. The Structure of Tensors

29 Strains that are not “wave compatible”
These two strains could not travel as a plane wave in 3-direction: with distance from the center the displacement would grow without limit, and a shear strain in the 13- and 23-planes would be enforced The Structure of Tensors

30 Three strains that are “wave compatible”
These three strains could travel as a plane wave in 3-direction without generating locally large displacements The plane shear strain (lowest example) could travel not only in 3-direction, but also in 1-direction The Structure of Tensors

31 All strains that are “wave compatible”in a given coordinate direction
Six mutually orthogonal unit strains Note that each shear strain could travel in two directions! The Structure of Tensors

32 The Structure of Tensors
All strains (as 6D-vectors) that are “wave compatible”in a given coordinate direction Six mutually orthogonal unit strains Note that each shear strain could travel in two directions! Of the two shear strains that can travel in 3-direction, one can also travel in 1-direction, the other also in 2-direction, etc. The Structure of Tensors

33 Symmetry planes and shear eigenstrains
The symmetry of a medium is controlled by its symmetry planes. Proposition: Two shear eigenstrains that share an axis define a symmetry plane perpendicular to this axis. Consider a set of six orthonormal eigenstrains, two of them plane shear strains in the 23- and 13- planes. It has the form The 12-plane is a symmetry plane if the set is invariant under a change of sign of the 3-axis, i.e. for elements with an even number of subscripts “3”, i.e., for all but the two shear strains. are arbitrary entries The two shear eigenstrains change sign, but for an eigenstrain this is irrelevant. The Structure of Tensors

34 Symmetry planes and shear waves
The symmetry of a medium is controlled by its symmetry planes A symmetry plane supports shear wave with cross-plane polar- ization in all direction. Conversely, a plane that does support these waves is a symmetry plane Two shear eigenstrains that share an axis thus define a symmetry plane perpendicular to this axis This holds for any two shear eigenstrains The Structure of Tensors

35 The Structure of Tensors
The equivalence set We had found that three of the 21 parameters describing an elastic tensor are “extraneous”: they describe not the tensor, but its orientation with respect to the “default” system (e.g., N–E–down) For a tensors without any symmetry plane that means that there is a three-parametric manifold of “equivalent” tensors that differ only in orientation. These are the elements of the “equivalence set”. If we construct a tensor with symmetry planes, we can choose the shear eigenstrains to let the symmetry planes coincide with the coordinate planes The Structure of Tensors

36 Equivalence for a single symmetry plane
Two shear eigentensors define a single plane of symmetry. Let the normal to this plane be the 3-axis. The 1- and 2-axis can have still any orientation in the symmetry plane, thus there is a 1-parametric manifold of equivalent tensors. This problem occurs with monoclinic and trigonal tensors, which have only one symmetry plane (but also with tetragonal tensors, where the plane orthogonal to the fourfold axis is regarded as the symmetry plane). We choose the orientation which gives the lowest number of stiffnesses. As far as elasticity is concerned, this is always possible. In a different (crystallographic) coordinate system, the number is higher (mono:12->13, trigo & tetra-> 6->7). The Structure of Tensors

37 Effect of one single shear eigenstrain
A single shear eigenstrain has no effect on symmetry, but a strong effect on the stiffness matrix. This orthonormal eigensystem leads to this Voigt stiffness matrix with 16 independent stiffnesses The A, B,…F are arbitrary positive numbers The black disks represent real numbers The tensor is stable “by design” The Structure of Tensors

38 Two shear eigenstrains -> monoclinic
Two shear eigenstrains generate a plane of symmetry, thus the tensor has “monoclinic” symmetry. This orthonormal eigensystem leads to this Voigt stiffness matrix with twelve independent stiffnesses The matrix on the right is automatically in the coordinate system by the two shear planes and the symmetry planes and therefore has twelve – not thirteen – stiffnesses. The Structure of Tensors

39 Three shear eigenstrains –> orthotropic
Three shear eigenstrains generate three planes of symmetry, thus the tensor has “orthotropic” symmetry. This orthonormal eigensystem leads to this Voigt stiffness matrix with nine independent stiffnesses Orthotropy marks an important point: up to now we had just to add new planes to increase the symmetry. Also, the “shape” of the matrix has reached its final form. From now on, co-planar shear tensors and identical eigenstiffnesses will be needed to increase symmetry. The Structure of Tensors

40 Example: Transverse Isotropy
TI is the anisotropy best known. On the other hand, the symmetry is high enough to give a good example of how additional symmetry planes depend on the eigensystem. The equatorial plane must be a symmetry plane. The eigenstiffnesses control the velocities of the waves with the appropriate in-plane shears along the three red lines. Thus the eigenstiffnesses must be identical. This makes the 3-axis at least a 4-fold axis. In addition we certainly have a shear eigenstrain in the 12-plane, since the two other shear planes are symmetry planes too. The Structure of Tensors

41 The eigensystem of Transverse Isotropy
To simplify the discussion, I determined with Mathematica the eigensystem of a general TI medium. I obtained for 1–4 Estff 2c c c c66 The Structure of Tensors

42 The eigensystem of TI: #5 and #6
p = c11 + (c33 - c66)/2, q = √[(p-c33)2 + 2c132]/2 Estff p – q p + q A A C 0 0 0 B B D 0 0 0 Each of the two tensors is orthogonal to the other four. To be orthogonal to each other, we need C.D = –2 A.B The Structure of Tensors

43 Overview of Eigensystems I
Eigensystems of monoclinic, orthotropic, and trigonal symmetry Capital letters: E plane shear; asterisk: d* isochoric strain The Structure of Tensors

44 Overview of Eigensystems II
Eigensystems of tetragonal, TI, cubic, and isotropic symmetry Capital letters: E plane shear; asterisk: d* isochoric strain Underlined: coplanar shear tensors The Structure of Tensors

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