Microstates of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry

Details Microstates of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry Microstates of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry

1998-05-21

arxiv.org/abs/hep-th/9805146v1

Phys.Rev.Lett.82:484-487,1999

Physics

High Energy Physics

High Energy Physics - Theory

11 pages, revtex

Scientific paper

10.1103/PhysRevLett.82.484

We show that a class of four-dimensional rotating black holes allow five-dimensional embeddings as black rotating strings. Their near-horizon geometry factorizes locally as a product of the three-dimensional anti-deSitter space-time and a two-dimensional sphere (AdS_3 x S^2), with angular momentum encoded in the global space-time structure. Following the observation that the isometries on the AdS_3 space induce a two-dimensional (super)conformal field theory on the boundary, we reproduce the microscopic entropy with the correct dependence on the black hole angular momentum.

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