Black Hole Entropy from BMS Symmetry at the Horizon
arXiv:1702.04439 · doi:10.1103/PhysRevLett.120.101301
Abstract
Near the horizon, the obvious symmetries of a black hole spacetime---the horizon-preserving diffeomorphisms---are enhanced to a larger symmetry group with a BMS algebra. Using dimensional reduction and covariant phase space techniques, I investigate this augmented symmetry, and show that it is strong enough to determine the black hole entropy.
11+1 pages; v2: added references; v3: introduction rewritten to provide more context
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