English

Black Hole Entropy and Soft Hair

High Energy Physics - Theory 2019-01-30 v4

Abstract

A set of infinitesimal VirasoroLVirasoroR{\rm Virasoro_{\,L}}\otimes{\rm 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 cL=cR=12Jc_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

Cite

@article{arxiv.1810.01847,
  title  = {Black Hole Entropy and Soft Hair},
  author = {Sasha Haco and Stephen W. Hawking and Malcolm J. Perry and Andrew Strominger},
  journal= {arXiv preprint arXiv:1810.01847},
  year   = {2019}
}

Comments

Accepted for publication by JHEP on 05/12/18