Quasi-Normal Modes of Brane-Localised Standard Model Fields

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dc.creatorKanti, P.
dc.creatorKonoplya, R. A.
dc.date2005-12-20
dc.date2006-01-23
dc.date.accessioned2026-07-07T10:45:32Z
dc.date.available2026-07-07T10:45:32Z
dc.descriptionWe present here a detailed study of the quasi-normal spectrum of brane-localised Standard Model fields in the vicinity of D-dimensional black-holes. A variety of such backgrounds (Schwarzschild, Reissner-Nordstrom and Schwarzszchild-(Anti) de Sitter) are investigated. The dependence of the quasi-normal spectra on the dimensionality D, spin of the field s, and multipole number l is analyzed. Analytical formulae are obtained for a number of limiting cases: in the limit of large multipole number for Schwarzschild, Schwarzschild-de Sitter and Reissner-Nordstrom black holes, in the extremal limit of the Schwarzschild-de Sitter black hole, and in the limit of small horizon radius in the case of Schwarzschild-Anti de Sitter black holes. We show that an increase in the number of hidden, extra dimensions results in the faster damping of all fields living on the brane, and that the localization of fields on a brane affects the QN spectrum in a number of additional ways, both direct and indirect.
dc.description13 pages, 4 figures, to be published in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-th/0512257
dc.identifierhttp://arxiv.org/abs/hep-th/0512257
dc.identifierPhys.Rev.D73:044002,2006
dc.identifierdoi:10.1103/PhysRevD.73.044002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182944
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasi-Normal Modes of Brane-Localised Standard Model Fields
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