Decay of Dirac Massive Hair in the Background of Spherical Black Hole

dc.creatorModerski, Rafał
dc.creatorRogatko, Marek
dc.date2008-05-06
dc.date.accessioned2026-07-07T11:50:35Z
dc.date.available2026-07-07T11:50:35Z
dc.descriptionThe intermediate and late-time behaviour of massive Dirac hair in the static spherically symmetric black hole spacetime was studied. It was revealed that the intermediate asymptotic pattern of decay of massive Dirac spinor hair is dependent on the mass of the field under consideration as well as the multiple number of the wave mode. The long-lived oscillatory tail observed at timelike infinity in the considered background decays slowly as t^{-5/6}.
dc.description8 pages, 5 figures, RevTex, to be published in Phys.Rev.D15
dc.identifierhttps://arxiv.org/abs/0805.0665
dc.identifierhttp://arxiv.org/abs/0805.0665
dc.identifierPhys.Rev.D77:124007,2008
dc.identifierdoi:10.1103/PhysRevD.77.124007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203603
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDecay of Dirac Massive Hair in the Background of Spherical Black Hole
dc.typetext

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