Object Picture of Quasinormal Modes for Stringy Black Holes

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dc.creatorXi, Ping
dc.creatorLi, Xin-zhou
dc.date2007-11-27
dc.date2007-12-20
dc.date.accessioned2026-07-07T11:54:23Z
dc.date.available2026-07-07T11:54:23Z
dc.descriptionWe study the quasinormal modes (QNMs) for stringy black holes. By using numerical calculation, the relations between the QNMs and the parameters of black holes are minutely shown. For (1+1)-dimensional stringy black hole, the real part of the quasinormal frequency increases and the imaginary part of the quasinormal frequency decreases as the mass of the black hole increases. Furthermore, the dependence of the QNMs on the charge of the black hole and the flatness parameter is also illustrated. For (1+3)-dimensional stringy black hole, increasing either the event horizon or the multipole index, the real part of the quasinormal frequency decreases. The imaginary part of the quasinormal frequency increases no matter whether the event horizon is increased or the multipole index is decreased.
dc.description4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0711.4193
dc.identifierhttp://arxiv.org/abs/0711.4193
dc.identifierChin.Phys.Lett.22:2763-2765,2005
dc.identifierdoi:10.1088/0256-307X/22/11/010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204882
dc.subjectHigh Energy Physics - Theory
dc.titleObject Picture of Quasinormal Modes for Stringy Black Holes
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