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arxiv: gr-qc/9806012 · v2 · pith:7EDDZPCSnew · submitted 1998-06-03 · 🌀 gr-qc · hep-th

Black holes, brick walls and the Boulware state

classification 🌀 gr-qc hep-th
keywords modelbekenstein-hawkingboulwarebrick-wallenergyentropylargereservations
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The brick-wall model seeks to explain the Bekenstein-Hawking entropy as a wall-contribution to the thermal energy of ambient quantum fields raised to the Hawking temperature. Reservations have been expressed concerning the self-consistency of this model. For example, it predicts large thermal energy densities near the wall, producing a substantial mass-correction and, presumably, a large gravitational back-reaction. We re-examine this model and conclude that these reservations are unfounded once the ground state---the Boulware state---is correctly identified. We argue that the brick-wall model and the Gibbons-Hawking instanton (which ascribes a topological origin to the Bekenstein-Hawking entropy) are mutually exclusive, alternative descriptions (complementary in the sense of Bohr) of the same physics.

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Cited by 2 Pith papers

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  2. Finite N Black Holes through the Brick Wall

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    Reinterprets the brick-wall model as an effective description of finite-N departures from the semiclassical near-horizon continuum in AdS/CFT, producing residual reflections and model-dependent echoes.