dc.contributorOkinawa Institute of Science and Technology
dc.contributorPerimeter Institute for Theoretical Physics
dc.contributorÉcole Polytechnique de Bruxelles
dc.contributorUniversity of Waterloo
dc.contributorUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-29T08:29:05Z
dc.date.accessioned2022-12-20T02:44:28Z
dc.date.available2022-04-29T08:29:05Z
dc.date.available2022-12-20T02:44:28Z
dc.date.created2022-04-29T08:29:05Z
dc.date.issued2020-12-11
dc.identifierPhysical Review Letters, v. 125, n. 24, 2020.
dc.identifier1079-7114
dc.identifier0031-9007
dc.identifierhttp://hdl.handle.net/11449/228879
dc.identifier10.1103/PhysRevLett.125.241302
dc.identifier2-s2.0-85098193365
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5409013
dc.description.abstractWe show that the gravitational phase space for the near-horizon region of a bifurcate, axisymmetric Killing horizon in any dimension admits a 2D conformal symmetry algebra with central charges proportional to the area. This extends the construction of Haco et. al. [J. High Energy Phys. 12 (2018) 098JHEPFG1029-847910.1007/JHEP12(2018)098] to generic Killing horizons appearing in solutions of Einstein's equations and motivates a holographic description in terms of a 2D conformal field theory. The Cardy entropy in such a field theory agrees with the Bekenstein-Hawking entropy of the horizon, suggesting a microscopic interpretation. A set of appendixes is included in the Supplemental Material that provides examples and further details of the calculations presented in the main text.
dc.languageeng
dc.relationPhysical Review Letters
dc.sourceScopus
dc.titleVirasoro Hair and Entropy for Axisymmetric Killing Horizons
dc.typeArtículos de revistas


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