| dc.creator | Bravo-Gaete, Moises | |
| dc.creator | Guajardo, Luis | |
| dc.creator | Mokhtar, Hassaine | |
| dc.date | 2017-09-07T18:53:55Z | |
| dc.date | 2017-09-07T18:53:55Z | |
| dc.date | 2017 | |
| dc.date.accessioned | 2019-11-20T15:07:08Z | |
| dc.date.available | 2019-11-20T15:07:08Z | |
| dc.identifier | http://repositorio.ucm.cl:8080/handle/ucm/121 | |
| dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/3031908 | |
| dc.description | 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. | |
| dc.language | en | |
| dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
| dc.source | Journal of High Energy Physics, 92, 1-25. | |
| dc.subject | Black holes | |
| dc.subject | Classical theories of gravity | |
| dc.title | A Cardy-like formula for rotating black holes with planar horizon | |
| dc.type | Artículos de revistas | |
