Black Hole Entropy without Brick Walls
J.- G. Demers, R. Lafrance, R.C. Myers

TL;DR
This paper confirms that black hole entropy can be derived from quantum field theory without the need for a brick wall cutoff, showing it matches the Bekenstein-Hawking formula and includes quantum corrections.
Contribution
It demonstrates that 't Hooft's statistical-mechanical approach reproduces the Bekenstein-Hawking entropy and accounts for quantum corrections without a brick wall.
Findings
Black hole entropy matches the Bekenstein-Hawking formula.
Quantum corrections arise from higher curvature terms.
No brick wall cutoff is necessary for entropy calculation.
Abstract
We present evidence which confirms a suggestion by Susskind and Uglum regarding black hole entropy. Using a Pauli-Villars regulator, we find that 't Hooft's approach to evaluating black hole entropy through a statistical-mechanical counting of states for a scalar field propagating outside the event horizon yields precisely the one-loop renormalization of the standard Bekenstein-Hawking formula, . Our calculation also yields a constant contribution to the black hole entropy, a contribution associated with the one-loop renormalization of higher curvature terms in the gravitational action.
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