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

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.

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

References in corpus (2)

• Holography, Thermodynamics and Fluctuations of Charged AdS Black Holes
• Late-Time Dynamics of Scalar Fields on Rotating Black Hole Backgrounds

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