Black Hole Evaporation and Large Extra Dimensions

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dc.creatorCasadio, Roberto
dc.creatorHarms, Benjamin
dc.date2000-04-02
dc.date2000-07-10
dc.date.accessioned2026-07-07T11:09:56Z
dc.date.available2026-07-07T11:09:56Z
dc.descriptionWe study the evaporation of black holes in space-times with extra dimensions of size L. We first obtain a potential which describes the expected behaviors of very large and very small black holes and then show that a (first order) phase transition, possibly signaled by an outburst of energy, occurs in the system when the horizon shrinks below L from a larger value. This is related to both a change in the topology of the horizon and the restoring of the translational symmetry along the extra dimensions.
dc.descriptionLaTeX with elsart.sty, 10 pages, 1 EPS figure. Replaced with final version to appear in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/hep-th/0004004
dc.identifierhttp://arxiv.org/abs/hep-th/0004004
dc.identifierPhys.Lett.B487:209-214,2000
dc.identifierdoi:10.1016/S0370-2693(00)00840-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190638
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Hole Evaporation and Large Extra Dimensions
dc.typetext

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