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Quasi-normal modes of the Kerr-Newman black hole

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Il Nuovo Cimento B (1971-1996)

Summary

The quasi-normal frequencies of the Kerr-Newman black hole are calculated using a well-known WKB semi-analytic method. It is the first time that quasi-normal frequencies for the Kerr-Newman black hole are ever calculated by any method. We consider perturbations with a frozen Maxwell field and a perturbed Einstein field. We were led to such a consideration, because, for combined perturbations of both fields, the equations do not decouple.

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Authors and Affiliations

  1. Department of Physics, Section Astrophysics, Astronomy and Mechanics, Aristotle University of Thessaloniki, 54006, Thessaloniki, Greece

    K. D. Kokkotas

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  1. K. D. Kokkotas
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Kokkotas, K.D. Quasi-normal modes of the Kerr-Newman black hole. Nuov Cim B 108, 991–998 (1993). https://doi.org/10.1007/BF02822861

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  • DOI: https://doi.org/10.1007/BF02822861

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