Mass and angular momenta of Kerr-anti-de Sitter spacetimes

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We briefly review how to compute the mass and angular momenta of rotating, asymptotically anti-de Sitter spacetimes in Einstein-Gauss-Bonnet theory of gravity using superpotentials derived from standard Noether identities. The calculations depend on the asymptotic form of the metrics only and hence take no account of the source of the curvature. When the source of curvature is a black hole, the results can be checked using the first law of black hole thermodynamics.
14th Workshop On General Relativity And Gravitation (JGRG 2004) 29 Nov - 3 Dec 2004, Kyoto, Japan

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/35204

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0502072
 http://arxiv.org/abs/gr-qc/0502072

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arXiv