Kerr black hole quasinormal frequencies

Details Kerr black hole quasinormal frequencies Kerr black hole quasinormal frequencies

2003-01-30

arxiv.org/abs/gr-qc/0301122v2

Phys.Rev. D67 (2003) 081501

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

3 pages, 2 figures

Scientific paper

10.1103/PhysRevD.67.081501

Black-hole quasinormal modes (QNM) have been the subject of much recent attention, with the hope that these oscillation frequencies may shed some light on the elusive theory of quantum gravity. We compare numerical results for the QNM spectrum of the (rotating) Kerr black hole with an {\it exact} formula Re$\omega \to T_{BH}\ln 3+\Omega m$, which is based on Bohr's correspondence principle. We find a close agreement between the two. Possible implications of this result to the area spectrum of quantum black holes are discussed.

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