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A detailed study of quasinormal frequencies of the Kerr black hole

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arxiv gr-qc/9610048 v1 pith:R7SLNMGE submitted 1996-10-22 gr-qc

Hisashi Onozawa (Tokyo Inst. of Tech.) This is my paper · ORCID
classification gr-qc
keywords frequenciesquasinormalkerrmethodonlyblackcontinuedfirst
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abstract

We compute the quasinormal frequencies of the Kerr black hole using a continued fraction method. The continued fraction method first proposed by Leaver is still the only known method stable and accurate for the numerical determination of the Kerr quasinormal frequencies. We numerically obtain not only the slowly but also the rapidly damped quasinormal frequencies and analyze the peculiar behavior of these frequencies at the Kerr limit. We also calculate the algebraically special frequency first identified by Chandrasekhar and confirm that it coincide with the $n=8$ quasinormal frequency only at the Schwarzschild limit.

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Cited by 5 Pith papers

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