Extended Symmetries at the Black Hole Horizon
Laura Donnay, Gaston Giribet, Hern\'an A. Gonz\'alez, Miguel Pino

TL;DR
This paper demonstrates that non-extremal black holes in four-dimensional general relativity have an infinite-dimensional symmetry algebra near the horizon, including supertranslations and Virasoro algebras, which relate to black hole entropy.
Contribution
It establishes a new infinite-dimensional symmetry structure at the black hole horizon and connects it to the Bekenstein-Hawking entropy, extending previous understanding of horizon symmetries.
Findings
Infinite-dimensional algebra of asymptotic Killing vectors at the horizon
Zero-mode charges reproduce black hole entropy
Simplified algebra and solutions in three-dimensional case
Abstract
We prove that non-extremal black holes in four-dimensional general relativity exhibit an infinite-dimensional symmetry in their near horizon region. By prescribing a physically sensible set of boundary conditions at the horizon, we derive the algebra of asymptotic Killing vectors, which is shown to be infinite-dimensional and includes, in particular, two sets of supertranslations and two mutually commuting copies of the Virasoro algebra. We define the surface charges associated to the asymptotic diffeomorphisms that preserve the boundary conditions and discuss the subtleties of this definition, such as the integrability conditions and the correct definition of the Dirac brackets. When evaluated on the stationary solutions, the only non-vanishing charges are the zero-modes. One of them reproduces the Bekenstein-Hawking entropy of Kerr black holes. We also study the extremal limit,…
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