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- W2045966188 abstract "Using series solutions and time-domain evolutions, we probe the eikonal limit of the gravitational and scalar-field quasinormal modes of large black holes and black branes in anti-de Sitter backgrounds. These results are particularly relevant for the AdS/CFT correspondence, since the eikonal regime is characterized by the existence of long-lived modes which (presumably) dominate the decay time scale of the perturbations. We confirm all the main qualitative features of these slowly damped modes as predicted by Festuccia and Liu [G. Festuccia and H. Liu, arXiv:0811.1033.] for the scalar-field (tensor-type gravitational) fluctuations. However, quantitatively we find dimensional-dependent correction factors. We also investigate the dependence of the quasinormal mode frequencies on the horizon radius of the black hole (brane) and the angular momentum (wave number) of vector- and scalar-type gravitational perturbations." @default.
- W2045966188 created "2016-06-24" @default.
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- W2045966188 date "2009-07-20" @default.
- W2045966188 modified "2023-09-23" @default.
- W2045966188 title "Quasinormal modes of black holes in anti-de Sitter space: A numerical study of the eikonal limit" @default.
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- W2045966188 doi "https://doi.org/10.1103/physrevd.80.024024" @default.
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