Evaporation of a black hole off of a tense brane

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dc.creatorDai, De-Chang
dc.creatorKaloper, Nemanja
dc.creatorStarkman, Glenn D.
dc.creatorStojkovic, Dejan
dc.date2006-11-16
dc.date2007-01-15
dc.date.accessioned2026-07-07T11:02:58Z
dc.date.available2026-07-07T11:02:58Z
dc.descriptionWe calculate the gray-body factors for scalar, vector and graviton fields in the background of an exact black hole localized on a tensional 3-brane in a world with two large extra dimensions. Finite brane tension modifies the standard results for the case with of a black hole on a brane with negligible tension. For a black hole of a fixed mass, the power carried away into the bulk diminishes as the tension increases, because the effective Planck constant, and therefore entropy of a fixed mass black hole, increase. In this limit, the semiclassical description of black hole decay becomes more reliable.
dc.descriptiona few typos corrected, accepted for publication in PRD
dc.identifierhttps://arxiv.org/abs/hep-th/0611184
dc.identifierhttp://arxiv.org/abs/hep-th/0611184
dc.identifierPhys.Rev.D75:024043,2007
dc.identifierdoi:10.1103/PhysRevD.75.024043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188433
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleEvaporation of a black hole off of a tense brane
dc.typetext

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