Intermediate Asymptotics of the Kerr Quasinormal Spectrum

Details Intermediate Asymptotics of the Kerr Quasinormal Spectrum Intermediate Asymptotics of the Kerr Quasinormal Spectrum

2005-05-23

arxiv.org/abs/gr-qc/0505112v1

Class.Quant.Grav. 22 (2005) L71-L76

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages

Scientific paper

10.1088/0264-9381/22/14/L01

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 \Omega, which is valid in the intermediate asymptotic regime 1<<\omega<<1/T_{BH}.

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