Quasinormal modes of Reissner-Nordstr$\ddot{o}$m Anti-de Sitter Black Holes

Details Quasinormal modes of Reissner-Nordstr$\ddot{o}$m Anti-de Sitter Black Holes Quasinormal modes of Reissner-Nordstr$\ddot{o}$m Anti-de Sitter Black Holes

2000-03-31

arxiv.org/abs/hep-th/0003295v1

Phys.Lett. B481 (2000) 79-88

Physics

High Energy Physics

High Energy Physics - Theory

14 pages, 8 figures, submitted to Phys. Lett. B

Scientific paper

10.1016/S0370-2693(00)00409-3

Complex frequencies associated with quasinormal modes for large Reissner-Nordstr$\ddot{o}$m Anti-de Sitter black holes have been computed. These frequencies have close relation to the black hole charge and do not linearly scale with the black hole temperature as in Schwarzschild Anti-de Sitter case. In terms of AdS/CFT correspondence, we found that the bigger the black hole charge is, the quicker for the approach to thermal equilibrium in the CFT. The properties of quasinormal modes for $l>0$ have also been studied.

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