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arxiv: gr-qc/0502083 · v3 · submitted 2005-02-21 · 🌀 gr-qc

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

classification 🌀 gr-qc
keywords 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

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.