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Semi-analytic expressions for quasinormal modes of slowly rotating Kerr black holes

We provide semi-analytic expressions for quasinormal mode frequencies of slowly rotating Kerr black holes to the quadratic order in the rotation parameter. We apply the parametrized black hole quasinormal mode ringdown formalism to the Chandrasekhar-Detweiler equation and the Sasaki-Nakamura equation instead of the Teukolsky equation, and compare our result with the previous numerical calculations.

preprint2020arXivOpen access
Yasuyuki HatsudaMasashi Kimura
gr-qc
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Open access2 authors1 topic
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Yasuyuki HatsudaMasashi Kimura

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