Bounding the greybody factors for Schwarzschild black holes

dc.creatorBoonserm, Petarpa
dc.creatorVisser, Matt
dc.date2008-06-13
dc.date2008-06-23
dc.date.accessioned2026-07-07T11:51:37Z
dc.date.available2026-07-07T11:51:37Z
dc.descriptionGreybody factors in black hole physics modify the naive Planckian spectrum that is predicted for Hawking radiation when working in the limit of geometrical optics. We consider the Schwarzschild geometry in (3+1) dimensions, and analyze the Regge-Wheeler equation for arbitrary particle spin S and wave-mode angular momentum L, deriving rigourous bounds on the greybody factors as a function of S, L, wave frequency (omega), and the black hole mass, m.
dc.description5 pages; revtex4; V2 - two references added
dc.identifierhttps://arxiv.org/abs/0806.2209
dc.identifierhttp://arxiv.org/abs/0806.2209
dc.identifierPhys.Rev.D78:101502,2008
dc.identifierdoi:10.1103/PhysRevD.78.101502
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203960
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleBounding the greybody factors for Schwarzschild black holes
dc.typetext

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