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Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background

Instituto de Física, Universidade de São Paulo, C.P. 66318, 05315-970, São Paulo-SP, Brazil

^*konoplya@fma.if.usp.br
^†zhidenko@fma.if.usp.br

Phys. Rev. D 76, 084018 – Published 17 October, 2007Erratum Phys. Rev. D 90, 029901 (2014)

DOI: https://doi.org/10.1103/PhysRevD.76.084018

Abstract

We find the quasinormal modes of the charged scalar and Dirac fields in the background of the rotating charged black holes, described by the Kerr-Newman-de Sitter solution. The dependence of the quasinormal spectrum upon the black hole parameters mass $M$ , angular momentum $a$ , charge $Q$ , as well as on values of the $Λ$ -term and a field charge $q$ is investigated. Special attention is given to the near extremal limit of the black hole charge. In particular, we find that for both scalar and Dirac fields, charged perturbations decay quicker for $q > 0$ and slower for $q < 0$ for values of black holes charge $Q$ less than some threshold value, which is close to the extremal value of charge and depend on parameters of the black holes.

Erratum

Erratum: Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background [Phys. Rev. D 76, 084018 (2007)]

R. A. Konoplya and A. Zhidenko

Phys. Rev. D 90, 029901 (2014)

Article Text

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Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background

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Erratum

Erratum: Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background [Phys. Rev. D 76, 084018 (2007)]

Article Text

References (17)

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