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Energy and Angular Momentum in D dimensional Kerr-AdS black holes-new formulation

Recently it was shown that the conserved charges of asymptotically anti de Sitter spacetimes can be written in an explicitly gauge-invariant way in terms of the linearized Riemann tensor and the Killing vectors. Here we employ this construction to compute the mass and angular momenta of the D dimensional Kerr-AdS black holes, which is one of the most remarkable Einstein metrics generalizing the four dimensional rotating black hole.

preprint2020arXivOpen access
Emel Altas
math-phmath.MPgr-qchep-th
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Emel Altas

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