A Cardy-like formula for rotating black holes with planar horizon
High Energy Physics - Theory
2017-04-19 v5
Abstract
We show that the semiclassical entropy of -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.
Keywords
Cite
@article{arxiv.1702.02416,
title = {A Cardy-like formula for rotating black holes with planar horizon},
author = {Moisés Bravo Gaete and Luis Guajardo and Mokhtar Hassaïne},
journal= {arXiv preprint arXiv:1702.02416},
year = {2017}
}
Comments
Published in JHEP04(2017)092