• Source: Symmetric tensor

In mathematics, a symmetric tensor is a tensor that is invariant under a permutation of its vector arguments:




T
(

v

1


,

v

2


,
…
,

v

r


)
=
T
(

v

σ
1


,

v

σ
2


,
…
,

v

σ
r


)


{\displaystyle T(v_{1},v_{2},\ldots ,v_{r})=T(v_{\sigma 1},v_{\sigma 2},\ldots ,v_{\sigma r})}


for every permutation σ of the symbols {1, 2, ..., r}. Alternatively, a symmetric tensor of order r represented in coordinates as a quantity with r indices satisfies





T


i

1



i

2


⋯

i

r




=

T


i

σ
1



i

σ
2


⋯

i

σ
r




.


{\displaystyle T_{i_{1}i_{2}\cdots i_{r}}=T_{i_{\sigma 1}i_{\sigma 2}\cdots i_{\sigma r}}.}


The space of symmetric tensors of order r on a finite-dimensional vector space V is naturally isomorphic to the dual of the space of homogeneous polynomials of degree r on V. Over fields of characteristic zero, the graded vector space of all symmetric tensors can be naturally identified with the symmetric algebra on V. A related concept is that of the antisymmetric tensor or alternating form. Symmetric tensors occur widely in engineering, physics and mathematics.




Definition


Let V be a vector space and




T
∈

V

⊗
k




{\displaystyle T\in V^{\otimes k}}


a tensor of order k. Then T is a symmetric tensor if





τ

σ


T
=
T



{\displaystyle \tau _{\sigma }T=T\,}


for the braiding maps associated to every permutation σ on the symbols {1,2,...,k} (or equivalently for every transposition on these symbols).
Given a basis {ei} of V, any symmetric tensor T of rank k can be written as




T
=

∑


i

1


,
…
,

i

k


=
1


N



T


i

1



i

2


⋯

i

k





e


i

1




⊗

e


i

2




⊗
⋯
⊗

e


i

k






{\displaystyle T=\sum _{i_{1},\ldots ,i_{k}=1}^{N}T_{i_{1}i_{2}\cdots i_{k}}e^{i_{1}}\otimes e^{i_{2}}\otimes \cdots \otimes e^{i_{k}}}


for some unique list of coefficients




T


i

1



i

2


⋯

i

k






{\displaystyle T_{i_{1}i_{2}\cdots i_{k}}}

(the components of the tensor in the basis) that are symmetric on the indices. That is to say





T


i

σ
1



i

σ
2


⋯

i

σ
k




=

T


i

1



i

2


⋯

i

k






{\displaystyle T_{i_{\sigma 1}i_{\sigma 2}\cdots i_{\sigma k}}=T_{i_{1}i_{2}\cdots i_{k}}}


for every permutation σ.
The space of all symmetric tensors of order k defined on V is often denoted by Sk(V) or Symk(V). It is itself a vector space, and if V has dimension N then the dimension of Symk(V) is the binomial coefficient




dim
⁡

Sym

k


⁡
(
V
)
=



(



N
+
k
−
1

k


)



.


{\displaystyle \dim \operatorname {Sym} ^{k}(V)={N+k-1 \choose k}.}


We then construct Sym(V) as the direct sum of Symk(V) for k = 0,1,2,...




Sym
⁡
(
V
)
=

⨁

k
=
0


∞



Sym

k


⁡
(
V
)
.


{\displaystyle \operatorname {Sym} (V)=\bigoplus _{k=0}^{\infty }\operatorname {Sym} ^{k}(V).}





Examples


There are many examples of symmetric tensors. Some include, the metric tensor,




g

μ
ν




{\displaystyle g_{\mu \nu }}

, the Einstein tensor,




G

μ
ν




{\displaystyle G_{\mu \nu }}

and the Ricci tensor,




R

μ
ν




{\displaystyle R_{\mu \nu }}

.
Many material properties and fields used in physics and engineering can be represented as symmetric tensor fields; for example: stress, strain, and anisotropic conductivity. Also, in diffusion MRI one often uses symmetric tensors to describe diffusion in the brain or other parts of the body.
Ellipsoids are examples of algebraic varieties; and so, for general rank, symmetric tensors, in the guise of homogeneous polynomials, are used to define projective varieties, and are often studied as such.
Given a Riemannian manifold



(
M
,
g
)


{\displaystyle (M,g)}

equipped with its Levi-Civita connection



∇


{\displaystyle \nabla }

, the covariant curvature tensor is a symmetric order 2 tensor over the vector space



V
=

Ω

2


(
M
)
=

⋀

2



T

∗


M


{\textstyle V=\Omega ^{2}(M)=\bigwedge ^{2}T^{*}M}

of differential 2-forms. This corresponds to the fact that, viewing




R

i
j
k
ℓ


∈
(

T

∗


M

)

⊗
4




{\displaystyle R_{ijk\ell }\in (T^{*}M)^{\otimes 4}}

, we have the symmetry




R

i
j

k
ℓ


=

R

k
ℓ

i
j




{\displaystyle R_{ij\,k\ell }=R_{k\ell \,ij}}

between the first and second pairs of arguments in addition to antisymmetry within each pair:




R

j
i
k
ℓ


=
−

R

i
j
k
ℓ


=

R

i
j
ℓ
k




{\displaystyle R_{jik\ell }=-R_{ijk\ell }=R_{ij\ell k}}

.




Symmetric part of a tensor


Suppose



V


{\displaystyle V}

is a vector space over a field of characteristic 0. If T ∈ V⊗k is a tensor of order



k


{\displaystyle k}

, then the symmetric part of



T


{\displaystyle T}

is the symmetric tensor defined by




Sym

T
=


1

k
!




∑

σ
∈



S



k





τ

σ


T
,


{\displaystyle \operatorname {Sym} \,T={\frac {1}{k!}}\sum _{\sigma \in {\mathfrak {S}}_{k}}\tau _{\sigma }T,}


the summation extending over the symmetric group on k symbols. In terms of a basis, and employing the Einstein summation convention, if




T
=

T


i

1



i

2


⋯

i

k





e


i

1




⊗

e


i

2




⊗
⋯
⊗

e


i

k




,


{\displaystyle T=T_{i_{1}i_{2}\cdots i_{k}}e^{i_{1}}\otimes e^{i_{2}}\otimes \cdots \otimes e^{i_{k}},}


then




Sym

T
=


1

k
!




∑

σ
∈



S



k





T


i

σ
1



i

σ
2


⋯

i

σ
k





e


i

1




⊗

e


i

2




⊗
⋯
⊗

e


i

k




.


{\displaystyle \operatorname {Sym} \,T={\frac {1}{k!}}\sum _{\sigma \in {\mathfrak {S}}_{k}}T_{i_{\sigma 1}i_{\sigma 2}\cdots i_{\sigma k}}e^{i_{1}}\otimes e^{i_{2}}\otimes \cdots \otimes e^{i_{k}}.}


The components of the tensor appearing on the right are often denoted by





T

(

i

1



i

2


⋯

i

k


)


=


1

k
!




∑

σ
∈



S



k





T


i

σ
1



i

σ
2


⋯

i

σ
k






{\displaystyle T_{(i_{1}i_{2}\cdots i_{k})}={\frac {1}{k!}}\sum _{\sigma \in {\mathfrak {S}}_{k}}T_{i_{\sigma 1}i_{\sigma 2}\cdots i_{\sigma k}}}


with parentheses () around the indices being symmetrized. Square brackets [] are used to indicate anti-symmetrization.




Symmetric product


If T is a simple tensor, given as a pure tensor product




T
=

v

1


⊗

v

2


⊗
⋯
⊗

v

r




{\displaystyle T=v_{1}\otimes v_{2}\otimes \cdots \otimes v_{r}}


then the symmetric part of T is the symmetric product of the factors:





v

1


⊙

v

2


⊙
⋯
⊙

v

r


:=


1

r
!




∑

σ
∈



S



r





v

σ
1


⊗

v

σ
2


⊗
⋯
⊗

v

σ
r


.


{\displaystyle v_{1}\odot v_{2}\odot \cdots \odot v_{r}:={\frac {1}{r!}}\sum _{\sigma \in {\mathfrak {S}}_{r}}v_{\sigma 1}\otimes v_{\sigma 2}\otimes \cdots \otimes v_{\sigma r}.}


In general we can turn Sym(V) into an algebra by defining the commutative and associative product ⊙. Given two tensors T1 ∈ Symk1(V) and T2 ∈ Symk2(V), we use the symmetrization operator to define:





T

1


⊙

T

2


=
Sym
⁡
(

T

1


⊗

T

2


)


(

∈

Sym


k

1


+

k

2




⁡
(
V
)

)

.


{\displaystyle T_{1}\odot T_{2}=\operatorname {Sym} (T_{1}\otimes T_{2})\quad \left(\in \operatorname {Sym} ^{k_{1}+k_{2}}(V)\right).}


It can be verified (as is done by Kostrikin and Manin) that the resulting product is in fact commutative and associative. In some cases the operator is omitted: T1T2 = T1 ⊙ T2.
In some cases an exponential notation is used:





v

⊙
k


=




v
⊙
v
⊙
⋯
⊙
v

⏟



k

times



=




v
⊗
v
⊗
⋯
⊗
v

⏟



k

times



=

v

⊗
k


.


{\displaystyle v^{\odot k}=\underbrace {v\odot v\odot \cdots \odot v} _{k{\text{ times}}}=\underbrace {v\otimes v\otimes \cdots \otimes v} _{k{\text{ times}}}=v^{\otimes k}.}


Where v is a vector.
Again, in some cases the ⊙ is left out:





v

k


=




v

v

⋯

v

⏟



k

times



=




v
⊙
v
⊙
⋯
⊙
v

⏟



k

times



.


{\displaystyle v^{k}=\underbrace {v\,v\,\cdots \,v} _{k{\text{ times}}}=\underbrace {v\odot v\odot \cdots \odot v} _{k{\text{ times}}}.}





Decomposition


In analogy with the theory of symmetric matrices, a (real) symmetric tensor of order 2 can be "diagonalized". More precisely, for any tensor T ∈ Sym2(V), there is an integer r, non-zero unit vectors v1,...,vr ∈ V and weights λ1,...,λr such that




T
=

∑

i
=
1


r



λ

i




v

i


⊗

v

i


.


{\displaystyle T=\sum _{i=1}^{r}\lambda _{i}\,v_{i}\otimes v_{i}.}


The minimum number r for which such a decomposition is possible is the (symmetric) rank of T. The vectors appearing in this minimal expression are the principal axes of the tensor, and generally have an important physical meaning. For example, the principal axes of the inertia tensor define the Poinsot's ellipsoid representing the moment of inertia. Also see Sylvester's law of inertia.
For symmetric tensors of arbitrary order k, decompositions




T
=

∑

i
=
1


r



λ

i




v

i


⊗
k




{\displaystyle T=\sum _{i=1}^{r}\lambda _{i}\,v_{i}^{\otimes k}}


are also possible. The minimum number r for which such a decomposition is possible is the symmetric rank of T. This minimal decomposition is called a Waring decomposition; it is a symmetric form of the tensor rank decomposition. For second-order tensors this corresponds to the rank of the matrix representing the tensor in any basis, and it is well known that the maximum rank is equal to the dimension of the underlying vector space. However, for higher orders this need not hold: the rank can be higher than the number of dimensions in the underlying vector space. Moreover, the rank and symmetric rank of a symmetric tensor may differ.




See also


Antisymmetric tensor
Ricci calculus
Schur polynomial
Symmetric polynomial
Transpose
Young symmetrizer




Notes






References


Bourbaki, Nicolas (1989), Elements of mathematics, Algebra I, Springer-Verlag, ISBN 3-540-64243-9.
Bourbaki, Nicolas (1990), Elements of mathematics, Algebra II, Springer-Verlag, ISBN 3-540-19375-8.
Greub, Werner Hildbert (1967), Multilinear algebra, Die Grundlehren der Mathematischen Wissenschaften, Band 136, Springer-Verlag New York, Inc., New York, MR 0224623.
Sternberg, Shlomo (1983), Lectures on differential geometry, New York: Chelsea, ISBN 978-0-8284-0316-0.




External links


Cesar O. Aguilar, The Dimension of Symmetric k-tensors

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• Tensor tegangan–energi
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