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Quasinormal modes of Reissner-Nordström black holes

Edward W. Leaver

  • Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109

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Phys. Rev. D 41, 2986 – Published 15 May, 1990Erratum Phys. Rev. D 43, 1434 (1991)

DOI: https://doi.org/10.1103/PhysRevD.41.2986

Abstract

We present a matrix-eigenvalue algorithm for accurately computing the quasinormal frequencies and modes of charged static black holes. The method is then refined through the introduction of a continued-fraction step. We believe the approach will generalize to a variety of nonseparable wave equations, including the Kerr-Newman case of charged rotating black holes.

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Erratum

Erratum: Quasinormal modes of Reissner-Nordström black holes

Edward W. Leaver
Phys. Rev. D 43, 1434 (1991)

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Phys. Rev. D 41, 2986– Published 15 May, 1990
  • Received 25 September 1989

© 1990 American Physical Society

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