ADM reduction of Einstein action and black hole entropy
I. Y. Park

TL;DR
This paper reduces the Einstein-Hilbert action to a lower-dimensional theory on a hypersurface, deriving black hole entropy and reproducing the Bekenstein-Hawking area law with subleading corrections.
Contribution
It introduces a novel reduction of the Einstein action to a hypersurface, resulting in a scalar theory that captures black hole entropy including quantum corrections.
Findings
Reproduces Bekenstein-Hawking entropy from hypersurface degrees of freedom
Derives a 2D Liouville type theory at the Schwarzschild radius
Identifies subleading logarithmic and inverse area corrections
Abstract
We reduce the 4D Einstein-Hilbert action to a constant-radius hypersurface of foliation. The resulting theory is a scalar theory defined on a 3D hypersurface of the original black hole background, and has an exponential potential. Once the the hypersurface is located at the Schwarzschild radius, the 3D theory is effectively reduced to a 2D Liouville type theory. We compute {the entropy associated with the hypersurface intrinsic degrees of freedom}, and show that its leading order reproduces the Bekenstein-Hawking area law. The subleading terms come in logarithm/inverse powers of the area.
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