Stability and thermodynamics of brane black holes

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dc.creatorAbdalla, E.
dc.creatorCuadros-Melgar, B.
dc.creatorPavan, A. B.
dc.creatorMolina, C.
dc.date2006-04-07
dc.date2006-08-27
dc.date.accessioned2026-07-07T07:09:37Z
dc.date.available2026-07-07T07:09:37Z
dc.descriptionWe consider scalar and axial gravitational perturbations of black hole solutions in brane world scenarios. We show that perturbation dynamics is surprisingly similar to the Schwarzschild case with strong indications that the models are stable. Quasinormal modes and late-time tails are discussed. We also study the thermodynamics of these scenarios verifying the universality of Bekenstein's entropy bound as well as the applicability of 't Hooft's brickwall method.
dc.description13 pages, 8 figures, published version
dc.identifierhttps://arxiv.org/abs/gr-qc/0604033
dc.identifierhttp://arxiv.org/abs/gr-qc/0604033
dc.identifierNucl.Phys. B752 (2006) 40-59
dc.identifierdoi:10.1016/j.nuclphysb.2006.06.017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111134
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleStability and thermodynamics of brane black holes
dc.typetext

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