Asymptotic black hole quasinormal frequencies

dc.creatorMotl, Lubos
dc.creatorNeitzke, Andrew
dc.date2003-01-23
dc.date2003-12-24
dc.date.accessioned2026-07-07T04:14:47Z
dc.date.available2026-07-07T04:14:47Z
dc.descriptionWe give a new derivation of the quasinormal frequencies of Schwarzschild black holes in d>=4 and Reissner-Nordstrom black holes in d=4, in the limit of infinite damping. For Schwarzschild in d>=4 we find that the asymptotic real part is T_Hawking.log(3) for scalar perturbations and for some gravitational perturbations; this confirms a result previously obtained by other means in the case d=4. For Reissner-Nordstrom in d=4 we find a specific generally aperiodic behavior for the quasinormal frequencies, both for scalar perturbations and for electromagnetic-gravitational perturbations. The formulae are obtained by studying the monodromy of the perturbation analytically continued to the complex plane; the analysis depends essentially on the behavior of the potential in the "unphysical" region near the black hole singularity.
dc.description21 pages, 4 EPS figures, JHEP3 LaTeX; v2: references added, typos corrected, discussion expanded; v3: references added, small changes, clarified relation between Schwarzschild and Reissner-Nordstrom asymptotic frequencies (published version of text)
dc.identifierhttps://arxiv.org/abs/hep-th/0301173
dc.identifierhttp://arxiv.org/abs/hep-th/0301173
dc.identifierAdv.Theor.Math.Phys. 7 (2003) 307-330
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51762
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymptotic black hole quasinormal frequencies
dc.typetext

Files

Collections