Intermediate Asymptotics of the Kerr Quasinormal Spectrum
arXiv:gr-qc/0505112 · doi:10.1088/0264-9381/22/14/L01
Abstract
We study analytically the quasinormal mode spectrum of near-extremal (rotating) Kerr black holes. We find an analytic expression for these black-hole resonances in terms of the black-hole physical parameters: its Bekenstein-Hawking temperature T_{BH} and its horizon's angular velocity Ω, which is valid in the intermediate asymptotic regime 1<<ω<<1/T_{BH}.
4 pages
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