Stability and Quasi Normal Modes of Charged Black Holes in Born-Infeld gravity

Details Stability and Quasi Normal Modes of Charged Black Holes in Born-Infeld gravity Stability and Quasi Normal Modes of Charged Black Holes in Born-Infeld gravity

2005-01-18

arxiv.org/abs/hep-th/0501138v4

Int.J.Theor.Phys. 45 (2006) 1630-1645

Physics

High Energy Physics

High Energy Physics - Theory

Latex, 17 pages, 13 figures, sections edited, references added. To appear in Inter.Jour. Theo. Phys

Scientific paper

In this paper we study the stability and the quasi normal modes of scalar perturbations of black holes. The static charged black hole considered here is a solution to Born-Infeld electrodynamics coupled to gravity. We conclude that the black hole is stable. We also compare the stability of it with the linear counter-part Reissner-Nordstrom black hole. The quasi normal modes are computed using the WKB method. The behavior of these modes with the non-linear parameter, temperature, mass of the scalar field and the spherical index are analyzed in detail.

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