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Black Holes of D=5 Supergravity

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arxiv hep-th/9810204 v2 pith:HLCLTYNY submitted 1998-10-25 hep-th astro-phgr-qc

J.P. Gauntlett , R.C. Myers , P.K. Townsend This is my paper · ORCID
classification hep-thastro-phgr-qc
keywords blackholesdiscussfeaturesnear-horizonsomesupergravitycauchy
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We discuss some general features of black holes of five-dimensional supergravity, such as the first law of black hole mechanics. We also discuss some special features of rotating supersymmetric black holes. In particular, we show that the horizon is a non-singular, and {\sl non-rotating}, null hypersurface whose intersection with a Cauchy surface is a squashed 3-sphere. We find the Killing spinors of the near-horizon geometry and thereby determine the near-horizon isometry supergroup.

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Cited by 5 Pith papers

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    Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.

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