Abstract
We prove that, in a space-time of dimension \(n>3\) with a velocity field that is shear-free, vorticity-free and acceleration-free, the covariant divergence of the Weyl tensor is zero if and only if the contraction of the Weyl tensor with the velocity is zero. This extends a property found in generalised Robertson–Walker spacetimes, where the velocity is also eigenvector of the Ricci tensor. Despite the simplicity of the statement, the proof is involved. As a product of the same calculation, we introduce a curvature tensor with an interesting recurrence property.
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26 September 2018
In our paper “A simple property of the Weyl tensor for a shear, vorticity and acceleration-free velocity field”.
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Appendix
Appendix
Proposition 4.4
In a twisted space the following identities hold among the Weyl tensor and the contracted Weyl tensor:
Proof
Contraction of (13) with \(u^j\) is:
Where possible, the vector \(u^k\) is taken inside covariant derivatives to take advantage of property (8)
Contraction with \(u^l\) yields the first result, (19):
which is used to replace the covariant divergences \(\nabla _p C_{jkl}{}^p\) in the previous expression
Some derivatives cancel, and we are left with
The final equation is obtained. \(\square \)
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Molinari, L.G., Mantica, C.A. A simple property of the Weyl tensor for a shear, vorticity and acceleration-free velocity field. Gen Relativ Gravit 50, 81 (2018). https://doi.org/10.1007/s10714-018-2398-9
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DOI: https://doi.org/10.1007/s10714-018-2398-9
Keywords
- Weyl tensor
- Twisted space-time
- Generalized Robertson–Walker spacetime
- Torse-forming vector
- Generalized curvature tensor