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

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

2002-07-04

arxiv.org/abs/gr-qc/0207028v3

Phys.Rev. D66 (2002) 084007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, LaTeX, 4 figures, considerable changes made and wrong interpretation of computations corrected

Scientific paper

10.1103/PhysRevD.66.084007

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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