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20 April 2024
 
  » arxiv » hep-th/9805146

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Microstates of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry
Mirjam Cvetic ; Finn Larsen ;
Date 22 May 1998
Journal Phys.Rev.Lett. 82 (1999) 484-487
Subject hep-th
AbstractWe 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.
Source arXiv, hep-th/9805146
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