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Gravito-Electromagnetic Perturbations and QNMs of Regular Black Holes

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arxiv 2210.00295 v2 pith:ZBV2SOSV submitted 2022-10-01 gr-qc

Gravito-Electromagnetic Perturbations and QNMs of Regular Black Holes

classification gr-qc
keywords blackholesperturbationsregularqnmscoupledelectromagneticequations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In the framework of Einstein's gravity coupled to nonlinear electromagnetic fields, we study gravito-electromagnetic perturbations of magnetic regular black holes. The master equations of perturbations are obtained through Chandrasekhar's procedure, in which gravitational perturbations with odd-parity are coupled to the electromagnetic perturbations with even-parity. As an application, we apply the master equations to obtain quasinormal modes (QNMs) for three types of regular black holes by using numerical method. Results show that QNMs of regular black holes depends significantly on the parameters of the theory and the magnetic charge of the black holes and are very different from that of the Reissner-Nordstr\"om black hole. Indications of these results on the stability of these regular black holes are discussed in detail.

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Cited by 2 Pith papers

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

  1. Grey-body factors of higher dimensional regular black holes in quasi-topological theories

    gr-qc 2026-01 unverdicted novelty 5.0

    Higher dimensional regular black holes in quasi-topological gravity have suppressed grey-body factors and Hawking radiation compared to singular black holes in general relativity.

  2. Grey-body factors of higher dimensional regular black holes in quasi-topological theories

    gr-qc 2026-01 unverdicted novelty 4.0

    Higher-dimensional regular black holes in quasi-topological gravity exhibit significantly suppressed grey-body factors and Hawking evaporation compared to singular black holes in general relativity.