Quasinormal modes of Kerr black holes: The determination of the quasinormal frequencies with a new technique

Details Quasinormal modes of Kerr black holes: The determination of the quasinormal frequencies with a new technique Quasinormal modes of Kerr black holes: The determination of the quasinormal frequencies with a new technique

2003-03-03

arxiv.org/abs/gr-qc/0303011v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, 4 figures, Revtex4 style

Scientific paper

We compute the quasinormal frequencies of rotating black holes using the continued fraction method first proposed by Leaver. The main difference with former works, is that our results are obtained by a new numerical technique which avoids the use of two dimensional root-finding routines. The technique is applied to evaluate the angular eigenvalues of Teukolsky's angular equation. This method allow us to calculate both the slowly and the rapidly damped quasinormal frequencies with excellent accuracy.

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