Black Hole Entropy from Bondi-Metzner-Sachs Symmetry at the Horizon

Carlip, S.

doi:10.1103/PhysRevLett.120.101301

Title: Black Hole Entropy from Bondi-Metzner-Sachs Symmetry at the Horizon

Journal Article · 08 March 2018 · Physical Review Letters

DOI: https://doi.org/10.1103/PhysRevLett.120.101301 · OSTI ID:1595482

Carlip, S. ^[1]

Univ. of California, Davis, CA (United States); Physics Department, University of California at Davis

Near the horizon, the obvious symmetries of a black hole spacetime—the horizon-preserving diffeomorphisms—are enhanced to a larger symmetry group with a BMS3 algebra. Using dimensional reduction and covariant phase space techniques, I explore this augmented symmetry, and demonstrate that it is strong enough to determine the black hole entropy.

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Research Organization:: Univ. of California, Davis, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)

Grant/Contract Number:: FG02-91ER40674

OSTI ID:: 1595482

Alternate ID(s):: OSTI ID: 1541290; OSTI ID: 1425234

Journal Information:: Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 10 Vol. 120; ISSN 0031-9007; ISSN PRLTAO

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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