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• W1530850497 abstract "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." @default.
• W1530850497 created "2016-06-24" @default.
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• W1530850497 date "1999-01-18" @default.
• W1530850497 modified "2023-10-12" @default.
• W1530850497 title "Statistical Entropy of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry" @default.
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• W1530850497 doi "https://doi.org/10.1103/physrevlett.82.484" @default.
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