paper

Quasinormal Modes of Bardeen Black Hole: Scalar Perturbations

arXiv:1208.5442 · doi:10.1103/PhysRevD.86.064039

Abstract

The purpose of this paper is to study quasinormal modes (QNM) of the Bardeen black hole due to scalar perturbations. We have done a thorough analysis of the QNM frequencies by varying the charge , mass and the spherical harmonic index . The unstable null geodesics are used to compute the QNM's in the eikonal limit. Furthermore, massive scalar field modes are also studied by varying the mass of the field. Comparisons are done with the QNM frequencies of the Reissner-Nordstrom black hole.

25 figures, Published in Physical Review D. Reference numbers corrected

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