Asymptotic quasinormal mode spectrum of rotating black holes

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dc.creatorHod, Shahar
dc.date2003-07-14
dc.date.accessioned2026-07-07T03:27:59Z
dc.date.available2026-07-07T03:27:59Z
dc.descriptionMotivated by novel results in the theory of black-hole quantization, we study {\it analytically} the quasinormal modes (QNM) of ({\it rotating}) Kerr black holes. The black-hole oscillation frequencies tend to the asymptotic value $ω_n=mΩ+i2πT_{BH}n$ in the $n \to \infty$ limit. This simple formula is in agreement with Bohr's correspondence principle. Possible implications of this result to the area spectrum of quantum black holes are discussed.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0307060
dc.identifierhttp://arxiv.org/abs/gr-qc/0307060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34651
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectCondensed Matter
dc.subjectHigh Energy Physics - Theory
dc.subjectQuantum Physics
dc.titleAsymptotic quasinormal mode spectrum of rotating black holes
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