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

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.

preprint2020arXivOpen access
Grigoris Panotopoulos
gr-qchep-th
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Grigoris Panotopoulos

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