Bekenstein-Hawking entropy from a phenomenological membrane

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dc.creatorGundlach, Carsten
dc.date1995-01-10
dc.date.accessioned2026-07-07T03:30:37Z
dc.date.available2026-07-07T03:30:37Z
dc.descriptionIt is pointed out that the entropy of a membrane which is quantized perturbatively around a background position of fixed radius in a black hole spacetime is equal to the Bekenstein-Hawking entropy, if 1) the membrane surface is the horizon surface plus one Planck unit, and 2) its temperature is the Hawking temperature. (This is a comment on gr-qc 9411037.)
dc.description1 journal page, Revtex
dc.identifierhttps://arxiv.org/abs/gr-qc/9501008
dc.identifierhttp://arxiv.org/abs/gr-qc/9501008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35583
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBekenstein-Hawking entropy from a phenomenological membrane
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