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Near Horizon Geometry of Rotating Black Holes in Five Dimensions | | Mirjam Cvetic
; Finn Larsen
; | | Date: |
19 May 1998 | | Journal: | Nucl.Phys. B531 (1998) 239-255 | | Subject: | hep-th | | 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. | | Source: | arXiv, hep-th/9805097 | | Services: | Forum | Review | PDF | Favorites | |
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