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Novel charged black hole solutions of Born-Infeld type: General properties, Smarr formula and Quasinormal frequencies

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arxiv 2304.09777 v1 pith:RXE7GWCN submitted 2023-04-19 gr-qc hep-th

L. Balart , S. Belmar-Herrera , G. Panotopoulos , Á. Rincón This is my paper · ORCID
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keywords quasinormalblackborn-infeldchargedformulamodelsnovelsmarr
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We investigate two novel models of charged black holes in the framework of non-linear electrodynamics of Born-Infeld type. In particular, starting from two concrete Lagrangian densities, the corresponding metric potentials, the electric field, the Smarr formula and finally, the (scalar) quasinormal modes are computed for each model. Our findings show that although the models look very similar, their quasinormal spectra are characterized by certain differences.

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Cited by 1 Pith paper

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  1. Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation

    gr-qc 2025-05 reject novelty 4.0 of 10

    The Kalb-Ramond black hole phenomenology is mostly an extension of known results, and its shadow formula is internally inconsistent, invalidating the EHT-based constraints.

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