Neutrino Quasinormal Modes of a Kerr-Newman-de Sitter Black Hole

dc.creatorChang, Jia-Feng
dc.creatorShen, You-Gen
dc.date2005-02-21
dc.date2005-03-26
dc.date.accessioned2026-07-07T10:48:18Z
dc.date.available2026-07-07T10:48:18Z
dc.descriptionUsing the Pöshl-Teller approximation, we evaluate the neutrino quasinormal modes (QNMs) of a Kerr-Newman-de Sitter black hole. The result shows that for a Kerr-Newman-de Sitter black hole, massless neutrino perturbation of large $Λ$, positive $m$ and small value of $n$ will decay slowly.
dc.description25 pages, 13 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0502083
dc.identifierhttp://arxiv.org/abs/gr-qc/0502083
dc.identifierNucl.Phys.B712:347-370,2005
dc.identifierdoi:10.1016/j.nuclphysb.2005.01.043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183828
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNeutrino Quasinormal Modes of a Kerr-Newman-de Sitter Black Hole
dc.typetext

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