A Cardy-like formula for rotating black holes with planar horizon
We show that the semiclassical entropy of D−dimensional rotating (an)isotropic black holes with planar horizon can be successfully computed according to a Cardy-like formula. This formula does not refer to any central charges but instead involves the vacuum energy which is identified with a gravi...
| Autor Principal: | Bravo-Gaete, Moises |
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| Otros Autores: | Guajardo, Luis, Mokhtar, Hassaine |
| Formato: | Artículo |
| Idioma: | English |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: |
http://repositorio.ucm.cl:8080/handle/ucm/121 |
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| Sumario: |
We show that the semiclassical entropy of D−dimensional rotating
(an)isotropic black holes with planar horizon can be successfully computed according to
a Cardy-like formula. This formula does not refer to any central charges but instead involves
the vacuum energy which is identified with a gravitational bulk soliton. The soliton
is obtained from the non-rotating black hole solution by means of a double analytic continuation.
The robustness of the Cardy-like formula is tested with numerous and varied
examples, including AdS, Lifshitz and hyperscaling violation planar black holes. |
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