Quasiparticle picture of black holes and the entropy--area relation

dc.creatorIizuka, Norihiro
dc.creatorKabat, Daniel
dc.creatorLifschytz, Gilad
dc.creatorLowe, David A.
dc.date2002-12-19
dc.date2003-01-06
dc.date.accessioned2026-07-07T11:32:08Z
dc.date.available2026-07-07T11:32:08Z
dc.descriptionWe propose an effective description of 0-brane black holes, in which the black hole is modeled as a gas of non-interacting quasi-particles in the dual quantum mechanics. This simple model is shown to account for many of the static thermodynamic properties of the black hole. It also accounts for dynamical properties, such as the rate at which energy gets thermalized by the black hole. We use the model to show that the entropy of the quantum mechanics is proportional to the black hole horizon area in Planck units.
dc.description20 pages, LaTeX, 2 eps figures. v2: references added
dc.identifierhttps://arxiv.org/abs/hep-th/0212246
dc.identifierhttp://arxiv.org/abs/hep-th/0212246
dc.identifierPhys.Rev.D67:124001,2003
dc.identifierdoi:10.1103/PhysRevD.67.124001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197493
dc.subjectHigh Energy Physics - Theory
dc.titleQuasiparticle picture of black holes and the entropy--area relation
dc.typetext

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