Topological Black Holes in Anti-de Sitter Space

Details Topological Black Holes in Anti-de Sitter Space Topological Black Holes in Anti-de Sitter Space

1998-08-06

arxiv.org/abs/hep-th/9808032v3

Class.Quant.Grav. 16 (1999) 1197-1205

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, Latex, v2 Computation of action corrected, conclusions unchanged, references added, v3 To appear in Classical and Qu

Scientific paper

10.1088/0264-9381/16/4/009

We consider a class of black hole solutions to Einstein's equations in d dimensions with a negative cosmological constant. These solutions have the property that the horizon is a (d-2)-dimensional Einstein manifold of positive, zero, or negative curvature. The mass, temperature, and entropy are calculated. Using the correspondence with conformal field theory, the phase structure of the solutions is examined, and used to determine the correct mass dependence of the Bekenstein-Hawking entropy.

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