Area spectrum of rotating black holes via the new interpretation of quasinormal modes

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dc.creatorVagenas, Elias C.
dc.date2008-04-21
dc.date2008-10-15
dc.date.accessioned2026-07-07T12:14:25Z
dc.date.available2026-07-07T12:14:25Z
dc.descriptionMotivated by the recent work on a new physical interpretation of quasinormal modes by Maggiore, we utilize this new proposal to the interesting case of Kerr black hole. In particular, by modifying Hod's idea, the resulting black hole horizon area is quantized and the resulting area quantum is in full agreement with Bekenstein's result. Furthermore, in an attempt to show that the area spectrum is equally spaced, we follow Kunstatter's method. We propose a new interpretation as a result of Maggiore's idea, for the frequency that appears in the adiabatic invariant of a black hole. The derived area spectrum is similar to that of the quantum-corrected Kerr black hole but it is not equally spaced.
dc.descriptionv1: 4 pages, REVTeX, no figures; v2: clarifications and comments added, comments on last result modified, Abstract slightly changed; v3: comments and references added;
dc.identifierhttps://arxiv.org/abs/0804.3264
dc.identifierhttp://arxiv.org/abs/0804.3264
dc.identifierJHEP0811:073,2008
dc.identifierdoi:10.1088/1126-6708/2008/11/073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211185
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleArea spectrum of rotating black holes via the new interpretation of quasinormal modes
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