Cotton tensor

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In differential geometry, the Cotton tensor on a (pseudo)-Riemannian manifold of dimension n is a third-order tensor concomitant of the metric, like the Weyl tensor. The concept is named after Émile Cotton. Just as the vanishing of the Weyl tensor for n ≥ 4 is a necessary and sufficient condition for the manifold to be conformally flat, the same is true for the Cotton tensor for n = 3, while for n < 3 it is identically zero.

In coordinates, and denoting the Ricci tensor by Rij and the scalar curvature by R, the components of the Cotton tensor are

C_{ijk} = \nabla_{k} R_{ij} - \nabla_{j} R_{ik} + \frac{1}{2(n-1)}\left( \nabla_{j}Rg_{ik} -  \nabla_{k}Rg_{ij}\right).

The Cotton tensor can be regarded as a vector valued 2-form, and for n=3 one can use the Hodge star operator to convert this in to a second order trace free tensor density

C_i^j = \nabla_{k} \left( R_{li} - \frac{1}{4} Rg_{li}\right)\epsilon^{klj},

sometimes called the Cotton–York tensor.

The proof of the classical result that for n = 3 the vanishing of the Cotton tensor is equivalent the metric being conformally flat is given by Eisenhart using a standard integrability argument. This tensor density is uniquely characterized by its conformal properties coupled with the demand that it be differentiable for arbitrary metrics, as shown by Aldersley.

Contents

[edit] Properties

[edit] Conformal rescaling

Under conformal rescaling of the metric \tilde{g} = e^{2\omega} g for some scalar function ω the Cotton-York tensor transforms as

 \tilde{C} = C \; - \; \operatorname{grad} \, \omega \; \lrcorner \; W,[citation needed]

where the gradient is plugged into the symmetric part of the Weyl tensor W.

[edit] Symmetries

The Cotton tensor has the following symmetries:

C_{ijk} = - C_{ikj} \,

and therefore

C_{[ijk]} = 0. \,

In addition the Bianchi formula for the Weyl tensor for can be rewritten as

\delta W = (3-n) C, \,

where δ is the positive divergence in the first component of W.

[edit] References

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