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arXiv · hep-th/0003295

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

Bin Wang·Chi-Yong Lin·Elcio Abdalla
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Abstract

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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Bin Wang, Chi-Yong Lin, Elcio Abdalla. 2000-03-31. Quasinormal modes of Reissner-Nordstr$\ddot{o}$m Anti-de Sitter Black Holes. https://doi.org/10.1016/s0370-2693(00)00409-3

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