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arxiv: gr-qc/0410025 · v2 · submitted 2004-10-06 · 🌀 gr-qc · astro-ph· hep-th

Quasinormal modes in time-dependent black hole background

Cheng-Gang Shao , Bin Wang , Elcio Abdalla , Ru-Keng Su This is my paper
classification 🌀 gr-qc astro-phhep-th
keywords blackholequasinormalbackgroundevolutionfieldmasslessmodes
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We have studied the evolution of the massless scalar field propagating in time-dependent charged Vaidya black hole background. A generalized tortoise coordinate transformation were used to study the evolution of the massless scalar field. It is shown that, for the slowest damped quasinormal modes, the approximate formulae in stationary Reissner-Nordstr\"{o}m black hole turn out to be a reasonable prescription, showing that results from quasinormal mode analysis are rather robust.

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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.