Neutrino Quasinormal Modes of a Kerr-Newman-de Sitter Black Hole
arXiv:gr-qc/0502083 · doi:10.1016/j.nuclphysb.2005.01.043
Abstract
Using 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 , positive and small value of will decay slowly.
25 pages, 13 figures
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Cited by in corpus (17)
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