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

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

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minor changes; accepted by CQG

Scientific paper

10.1088/0264-9381/22/2/013

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.

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