Adaptively Refined Large-Eddy Simulations of Galaxy Clusters

Appendix B Properties of second order tensors

A second order tensor can be decomposed into a symmetric and an antisymmetric part in the following way

Ti⁢j=12⁢(Ti⁢j+Tj⁢i)⏟symmetric+12⁢(Ti⁢j-Tj⁢i)⏟antisymmetric. (B.1)

It can also be decomposed into an isotropic and deviatoric part by subtracting and adding the trace of the tensor like

Ti⁢j=1n⁢δi⁢j⁢Tk⁢k⏟isotropic+Ti⁢j-1n⁢δi⁢j⁢Tk⁢k⏟deviatoric, tracefree. (B.2)

Combining these two relations yields the general decomposition

Ti⁢j=1n⁢δi⁢j⁢Tk⁢k⏞isotropic+12⁢(Ti⁢j+Tj⁢i-2n⁢δi⁢j⁢Tk⁢k)⏟symmetric, tracefree+12⁢(Ti⁢j-Tj⁢i)⏞deviatoric, tracefree⏟symmetric⁢⏟ antisymmetric. (B.3)

An interesting relation can be found when computing the contraction of a unsymmetric tensor Ui⁢j≠Uj⁢i with a symmetric tensor Vi⁢j=Vj⁢i

Ui⁢j⁢Vi⁢j=12⁢Ui⁢j⁢Vi⁢j+12⁢Uj⁢i⁢Vj⁢i=12⁢Ui⁢j⁢Vi⁢j+12⁢Uj⁢i⁢Vi⁢j=12⁢(Ui⁢j+Uj⁢i)⁢Vi⁢j. (B.4)

In analogy one finds for the contraction of an unsymmetric tensor Ui⁢j with an antisymmetric tensor Wi⁢j=-Wj⁢i

Ui⁢j⁢Wi⁢j=12⁢(Ui⁢j-Uj⁢i)⁢Wi⁢j. (B.5)