Abstract
We show that the gravitational phase space for the near-horizon region of a bifurcate, axisymmetric Killing horizon in any dimension admits a 2D conformal symmetry algebra with central charges proportional to the area. This extends the construction of Haco et. al. [J. High Energy Phys. 12 (2018) 098JHEPFG1029-847910.1007/JHEP12(2018)098] to generic Killing horizons appearing in solutions of Einstein's equations and motivates a holographic description in terms of a 2D conformal field theory. The Cardy entropy in such a field theory agrees with the Bekenstein-Hawking entropy of the horizon, suggesting a microscopic interpretation. A set of appendixes is included in the Supplemental Material that provides examples and further details of the calculations presented in the main text.
Highlights
We show that the gravitational phase space for the near-horizon region of a bifurcate, axisymmetric Killing horizon in any dimension admits a 2D conformal symmetry algebra with central charges proportional to the area
Carlip in particular demonstrated that the conformal symmetries were not special to AdS3 black holes; rather, they arise for generic Killing horizons
As a by-product, it motivated a different choice of near-horizon symmetry generators whose periodicities followed from the rotational symmetry of the Kerr black hole, thereby resolving one issue in Carlip’s original construction [22,23]
Summary
We show that the gravitational phase space for the near-horizon region of a bifurcate, axisymmetric Killing horizon in any dimension admits a 2D conformal symmetry algebra with central charges proportional to the area. 12 (2018) 098] to generic Killing horizons appearing in solutions of Einstein’s equations and motivates a holographic description in terms of a 2D conformal field theory. Carlip in particular demonstrated that the conformal symmetries were not special to AdS3 black holes; rather, they arise for generic Killing horizons.
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