On the mass of a Kerr-anti-de Sitter spacetime in D dimensions

Abstract

We show how to compute the mass of a Kerr-anti-de Sitter spacetime with respect to the anti-de Sitter background in any dimension, using a superpotential which has been derived from standard Noether identities. The calculation takes no account of the source of the curvature and confirms results obtained for black holes via the first law of thermodynamics.

minor changes; accepted by CQG

References in corpus (1)

• Relativistic conservation laws and integral constraints for large cosmological perturbations

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