The Mystery of the Asymptotic Quasinormal Modes of Gauss-Bonnet Black Holes

dc.creatorDaghigh, R. G.
dc.creatorKunstatter, G.
dc.creatorZiprick, J.
dc.date2006-11-27
dc.date.accessioned2026-07-07T11:01:27Z
dc.date.available2026-07-07T11:01:27Z
dc.descriptionWe analyze the quasinormal modes of $D$-dimensional Schwarzschild black holes with the Gauss-Bonnet correction in the large damping limit and show that standard analytic techniques cannot be applied in a straightforward manner to the case of infinite damping. However, by using a combination of analytic and numeric techniques we are able to calculate the quasinormal mode frequencies in a range where the damping is large but finite. We show that for this damping region the famous $\ln(3)$ appears in the real part of the quasinormal mode frequency. In our calculations, the Gauss-Bonnet coupling, $α$, is taken to be much smaller than the parameter $μ$, which is related to the black hole mass.
dc.description12 pages and 5 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0611139
dc.identifierhttp://arxiv.org/abs/gr-qc/0611139
dc.identifierClass.Quant.Grav.24:1981-1992,2007
dc.identifierdoi:10.1088/0264-9381/24/8/005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187958
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Mystery of the Asymptotic Quasinormal Modes of Gauss-Bonnet Black Holes
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