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

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arxiv hep-th/0003295 v1 pith:JVNLTOCA submitted 2000-03-31 hep-th

classification hep-th
keywords blackanti-deholemodesquasinormalsitterbeencharge
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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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  1. Quasinormal modes response to thermodynamic phase transitions in the charged AdS black hole surrounded by perfect fluid dark matter

    gr-qc 2026-08 conditional novelty 4.0 of 10

    In charged AdS black holes surrounded by perfect fluid dark matter, the fundamental scalar quasinormal mode jumps between two branches at the first-order small/large black hole transition, stays smooth at the critical...

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