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

Abstract

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.

Reference added. It belongs to Axioms' Special Issue: "Theory and Mathematical Aspects of Black Holes". It contains material from arXiv:1711.04146, arXiv:1904.10847, arXiv:1910.08538

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• Shadows and weak gravitational lensing by the black hole in Einstein-Maxwell-scalar theory
• Quasinormal modes of black holes with a scalar hair in Einstein-Maxwell-dilaton theory
• Optical features of AdS black holes in the novel 4D Einstein-Gauss-Bonnet gravity coupled to nonlinear electrodynamics
• Radiation properties of the accretion disk around a black hole in Einstein-Maxwell-scalar theory
• Novel charged black hole solutions of Born-Infeld type: General properties, Smarr formula and Quasinormal frequencies
• Thermodynamics and Quasinormal Modes of the Dymnikova Black Hole in Higher Dimensions
• Black Holes with Abelian and Non-Abelian Charges and Their Impact on Matter Accretion Flows
• Three-dimensional slowly rotating black hole in Einstein-power-Maxwell theory