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.
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Gaete, M.B., Guajardo, L. & Hassaïne, M. A Cardy-like formula for rotating black holes with planar horizon. J. High Energ. Phys. 2017, 92 (2017). https://doi.org/10.1007/JHEP04(2017)092
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DOI: https://doi.org/10.1007/JHEP04(2017)092