A Cardy-like formula for rotating black holes with planar horizon

dc.contributor.author	Bravo-Gaete, Moises
dc.contributor.author	Guajardo, Luis
dc.contributor.author	Mokhtar, Hassaine
dc.date.accessioned	2017-09-07T18:53:55Z
dc.date.available	2017-09-07T18:53:55Z
dc.date.issued	2017
dc.identifier.uri	http://repositorio.ucm.cl/handle/ucm/121
dc.description.abstract	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.	es_CL
dc.language.iso	en	es_CL
dc.rights	Atribución-NoComercial-SinDerivadas 3.0 Chile	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/cl/	*
dc.source	Journal of High Energy Physics, 92, 1-25.	es_CL
dc.subject	Black holes	es_CL
dc.subject	Classical theories of gravity	es_CL
dc.title	A Cardy-like formula for rotating black holes with planar horizon	es_CL
dc.type	Article	es_CL
dc.ucm.facultad	Facultad de Ciencias Básicas	es_CL
dc.ucm.indexacion	Scopus	es_CL
dc.ucm.indexacion	Isi	es_CL