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• W3100453485 abstract "We provide a classification of near-horizon geometries of supersymmetric, asymptotically antide Sitter, black holes of five-dimensional U(1) 3 -gauged supergravity which admit two rotational symmetries. We find three possibilities: a topologically spherical horizon, an S 1 × S 2 horizon and a toroidal horizon. The near-horizon geometry of the topologically spherical case turns out to be that of the most general known supersymmetric, asymptotically anti-de Sitter, black hole of U(1) 3 -gauged supergravity. The other two cases have constant scalars and only exist in particular regions of this moduli space – in particular they do not exist within minimal gauged supergravity. We also find a solution corresponding to the near-horizon geometry of a threecharge supersymmetric black ring held in equilibrium by a conical singularity; when lifted to type IIB supergravity this solution can be made regular, resulting in a discrete family of warped AdS3 geometries. Analogous results are presented in U(1) n gauged supergravity." @default.
• W3100453485 created "2020-11-23" @default.
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• W3100453485 date "2007-12-04" @default.
• W3100453485 modified "2023-10-14" @default.
• W3100453485 title "Near-horizon geometries of supersymmetric<i>AdS</i>₅black holes" @default.
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• W3100453485 doi "https://doi.org/10.1088/1126-6708/2007/12/015" @default.
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