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arXiv · hep-th/9805097

Near Horizon Geometry of Rotating Black Holes in Five Dimensions

Mirjam Cvetic·Finn Larsen
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Abstract

We interpret the general rotating black holes in five dimensions as rotating black strings in six dimensions. In the near horizon limit the geometry is locally AdS_3 x S_3, as in the nonrotating case. However, the global structure couples the AdS_3 and the S_3, giving angular velocity to the S_3. The asymptotic geometry is exploited to count the microstates and recover the precise value of the Bekenstein- Hawking entropy, with rotation taken properly into account. We discuss the perturbation spectrum of the rotating black hole, and its relation to the underlying conformal field theory.

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Mirjam Cvetic, Finn Larsen. 1998-05-18. Near Horizon Geometry of Rotating Black Holes in Five Dimensions. https://doi.org/10.1016/s0550-3213(98)00604-x

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