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Journal of High Energy Physics

, 2017:92

First Online: 18 April 2017Received: 13 February 2017Accepted: 10 April 2017DOI: 10.1007-JHEP042017092

Cite this article as: Gaete, M.B., Guajardo, L. & Hassaïne, M. J. High Energ. Phys. 2017 2017: 92. doi:10.1007-JHEP042017092 Abstract

We show that the semiclassical entropy of D−dimensional rotating anisotropic 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.

KeywordsBlack Holes Classical Theories of Gravity ArXiv ePrint: 1702.02416

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Autor: Moisés Bravo Gaete - Luis Guajardo - Mokhtar Hassaïne

Fuente: https://link.springer.com/

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