Second Order Perturbative Calculation of Quasinormal Modes of Schwarzschild Black Holes

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dc.creatorKao, Hsien-chung
dc.date2007-04-02
dc.date.accessioned2026-07-07T10:20:14Z
dc.date.available2026-07-07T10:20:14Z
dc.descriptionWe analytically calculate to second order the correction to the asymptotic form of quasinormal frequencies of four dimensional Schwarzschild black holes based on the monodromy analysis proposed by Motl and Neitzke. Our results are in good agreement with those obtained from numerical calculation.
dc.description12 pages, LaTex
dc.identifierhttps://arxiv.org/abs/0704.0284
dc.identifierhttp://arxiv.org/abs/0704.0284
dc.identifierPhys.Rev.D75:124008,2007
dc.identifierdoi:10.1103/PhysRevD.75.124008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/174783
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSecond Order Perturbative Calculation of Quasinormal Modes of Schwarzschild Black Holes
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