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Quasinormal modes of charged black holes in higher-dimensional Einstein-power-Maxwell theory

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arxiv 2005.08338 v2 pith:CK4Y66HU submitted 2020-05-17 gr-qc hep-th

Grigoris Panotopoulos This is my paper · ORCID
classification gr-qchep-th
keywords blackholesquasinormalchargedeinstein-power-maxwellscalartheoryangular
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We compute the quasinormal frequencies for scalar perturbations of charged black holes in five-dimensional Einstein-power-Maxwell theory. The impact on the spectrum of the electric charge of the black holes, of the angular degree, of the overtone number, and of the mass of the test scalar field is investigated in detail. The quasinormal spectra in the eikonal limit are computed as well for several different space-time dimensionalities.

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  1. Quasinormal modes of a quantum inspired black hole in four dimensions with cosmological constant

    gr-qc 2026-07 conditional novelty 6.0 of 10

    Quasinormal frequencies for scalar and Dirac perturbations of a Kazakov-Solodukhin-type quantum black hole with Lambda are computed by WKB and characteristic integration; all modes are stable and the quantum parameter...

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