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 · Fri Mar 09 00:00:00 EST 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)

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)

Grant/Contract Number:: FG02-91ER40674

OSTI ID:: 1595482

Alternate ID(s):: OSTI ID: 1425234

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

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 42 works

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Black Hole Entropy and Soft Hair Haco, Sasha; Hawking, Stephen W.; Perry, Malcolm J. arXiv https://doi.org/10.48550/arxiv.1810.01847	text	January 2018
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A fuzzy bipolar celestial sphere Alessio, Francesco; Arzano, Michele arXiv https://doi.org/10.48550/arxiv.1901.01167	text	January 2019
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