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arxiv: gr-qc/0207028 · v3 · submitted 2002-07-04 · 🌀 gr-qc

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Decay of charged scalar field around a black hole: quasinormal modes of R-N, R-N-AdS and dilaton black holes

R.A.Konoplya
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classification 🌀 gr-qc
keywords blackchargeddecayneutralperturbationsdilatonholeholes
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It is well known that the charged scalar perturbations of the Reissner-Nordstrom metric will decay slower at very late times than the neutral ones, thereby dominating in the late time signal. We show that at the stage of quasinormal ringing, on the contrary, the neutral perturbations will decay slower for RN, RNAdS and dilaton black holes. The QN frequencies of the nearly extreme RN black hole have the same imaginary parts (damping times) for charged and neutral perturbations. An explanation of this fact is not clear but, possibly, is connected with the Choptuik scaling.

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Cited by 2 Pith papers

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    Increasing the mass of a perturbing scalar field around Einstein-Maxwell-dilaton black holes strongly suppresses damping in several quasinormal branches, producing quasi-resonant long-lived oscillations.

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

    gr-qc 2011-02 accept novelty 1.0

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