Quasinormal modes and second order thermodynamic phase transition for Reissner-Nordström black hole

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dc.creatorJing, Jiliang
dc.creatorPan, Qiyuan
dc.date2008-02-01
dc.date.accessioned2026-07-07T11:40:04Z
dc.date.available2026-07-07T11:40:04Z
dc.descriptionThe relation between the quasinormal modes (QNMs) and the second order thermodynamic phase transition (SOTPT) for the Reissner-Nordström (RN) black hole is studied. It is shown that the quasinormal frequencies of the RN black hole start to get a spiral-like shape in the complex $ω$ plane and both the real and imaginary parts become the oscillatory functions of the charge if the real part of the quasinormal frequencies arrives at its maximum at the second order phase transition point of Davies for given overtone number and angular quantum number. That is to say, we can find out the SOTPT point from the QNMs of the RN black hole. The fact shows that the quasinormal frequencies carry the thermodynamical information of the RN black hole.
dc.description10 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0802.0043
dc.identifierhttp://arxiv.org/abs/0802.0043
dc.identifierPhys.Lett.B660:13-18,2008
dc.identifierdoi:10.1016/j.physletb.2007.11.039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200145
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleQuasinormal modes and second order thermodynamic phase transition for Reissner-Nordström black hole
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