Black hole entropy and soft hair
Open Access
- 17 December 2018
- journal article
- research article
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2018 (12) , 98
Abstract
A set of infinitesimal Virasoro L ⊗ Virasoro R diffeomorphisms are presented which act non-trivially on the horizon of a generic Kerr black hole with spin J. The covariant phase space formalism provides a formula for the Virasoro charges as surface integrals on the horizon. Integrability and associativity of the charge algebra are shown to require the inclusion of ‘Wald-Zoupas’ counterterms. A counterterm satisfying the known consistency requirement is constructed and yields central charges c L = c R = 12J. Assuming the existence of a quantum Hilbert space on which these charges generate the symmetries, as well as the applicability of the Cardy formula, the central charges reproduce the macroscopic area-entropy law for generic Kerr black holes.Keywords
All Related Versions
This publication has 85 references indexed in Scilit:
- Conformal symmetry for black holes in four dimensionsJournal of High Energy Physics, 2012
- New theoretical approaches to black holesNew Astronomy Reviews, 2008
- AdS3 black holes and a stringy exclusion principleJournal of High Energy Physics, 1998
- Black hole entropy from near-horizon microstatesJournal of High Energy Physics, 1998
- Statistical Hair on Black HolesPhysical Review Letters, 1996
- Counting States of Near-Extremal Black HolesPhysical Review Letters, 1996
- Comparison of the Noether charge and Euclidean methods for computing the entropy of stationary black holesPhysical Review D, 1995
- Quasilocal energy and conserved charges derived from the gravitational actionPhysical Review D, 1993
- Local symmetries and constraintsJournal of Mathematical Physics, 1990
- Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravityCommunications in Mathematical Physics, 1986