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Quasinormal modes of charged black holes with corrections from nonlinear electrodynamics

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arxiv 2111.06273 v2 pith:F2QA5XRU submitted 2021-11-11 gr-qc hep-th

classification gr-qchep-th
keywords quasinormalelectrodynamicscorrectionsmodesnonlinearblackchargedcoefficients
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We study quasinormal modes related to gravitational and electromagnetic perturbations of spherically symmetric charged black holes in nonlinear electrodynamics. Beyond the linear Maxwell electrodynamics, we consider a class of Lagrangian with higher-order corrections written by the electromagnetic field strength and its Hodge dual with arbitrary coefficients, and we parametrize the corrections for quasinormal frequencies in terms of the coefficients. It is confirmed that the isospectrality of quasinormal modes under parity is generally violated due to nonlinear electrodynamics. As applications, the corrections for quasinormal frequencies in Euler-Heisenberg and Born-Infeld electrodynamics are calculated, then it is clarified that the nonlinear effects act to lengthen the oscillation period and enhance the damping rate of the quasinormal modes.

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Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Resonance of black hole quasinormal modes in coupled systems

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    A new basis-invariant excitation factor for coupled black hole perturbation systems shows resonant amplification at avoided crossings between fundamental modes of different fields in the Einstein-Maxwell-axion theory.

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  5. Causality Constraints on Black Hole Thermodynamics in Nonlinear Electrodynamics

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    Causality in nonlinear electrodynamics forces the entropy-to-mass-squared ratio of black holes to decrease with mass and the extremal mass-to-charge ratio to increase with charge.

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    A rotating Yang-Mills charged black hole surrounded by perfect fluid dark matter is shown to have a smaller and more distorted shadow as the dark matter parameter increases, with EHT-derived bounds on the dark matter ...

  7. Quasinormal Modes of Schwarzschild Black Holes in the Dehnen-(1, 4, 5/2) Type Dark Matter Halos

    gr-qc 2025-05 reject novelty 4.0 of 10

    Quasinormal mode frequencies of a Schwarzschild black hole in a Dehnen-(1,4,5/2) dark matter halo are computed and found to decrease as halo density or core radius increases, with stability preserved.

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