On area and entropy of a black hole

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dc.creatorAlekseev, A.
dc.creatorPolychronakos, A. P.
dc.creatorSmedbäck, M.
dc.date2000-04-06
dc.date.accessioned2026-07-07T11:09:56Z
dc.date.available2026-07-07T11:09:56Z
dc.descriptionWe consider a model of a black hole consisting of a number of elementary components. Examples of such models occur in the Ashtekar's approach to canonical Quantum Gravity and in M-theory. We show that treating the elementary components as completely distinguishable leads to the area law for the black hole entropy. Contrary to previous results, we show that no Bose condensation occurs, the area has big local fluctuations and that in the framework of canonical Quantum Gravity the area of the black hole horizon is equidistantly quantized.
dc.descriptionLaTeX, 4 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0004036
dc.identifierhttp://arxiv.org/abs/hep-th/0004036
dc.identifierPhys.Lett.B574:296-300,2003
dc.identifierdoi:10.1016/j.physletb.2003.08.062
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190639
dc.subjectHigh Energy Physics - Theory
dc.titleOn area and entropy of a black hole
dc.typetext

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