Quasinormal modes of Reissner-Nordstr$\ddot{o}$m Anti-de Sitter Black Holes
arXiv:hep-th/0003295 · doi:10.1016/S0370-2693(00)00409-3
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