Asymptotic quasinormal mode spectrum of rotating black holes

Details Asymptotic quasinormal mode spectrum of rotating black holes Asymptotic quasinormal mode spectrum of rotating black holes

2003-07-14

arxiv.org/abs/gr-qc/0307060v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages

Scientific paper

Motivated 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 $\omega_n=m\Omega+i2\pi T_{BH}n$ 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.

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