paper

Near-Horizon BMS Symmetry, Dimensional Reduction, and Black Hole Entropy

arXiv:1910.01762 · doi:10.1103/PhysRevD.101.046002

Abstract

In an earlier short paper [Phys.\ Rev.\ Lett.\ 120 (2018) 101301, arXiv:1702.04439], I argued that the horizon-preserving diffeomorphisms of a generic black hole are enhanced to a larger BMS symmetry, which is powerful enough to determine the Bekenstein-Hawking entropy. Here I provide details and extensions of that argument, including a loosening of horizon boundary conditions and a more thorough treatment of dimensional reduction and meaning of a "near-horizon symmetry."

28 pages; longer, more detailed (and extended) version of arXiv:1702.04439

References in corpus (7)

Cited by in corpus (18)