Neutrino Quasinormal Modes of a Kerr-Newman-de Sitter Black Hole
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🌀 gr-qc
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blackholekerr-newman-deneutrinosittermodesquasinormalapproximation
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Using the P\"{o}shl-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 $\Lambda$, positive $m$ and small value of $n$ will decay slowly.
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Cited by 1 Pith paper
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Quasinormal modes of black holes: from astrophysics to string theory
This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.
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