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Existence of Reissner-Nordstrom type black holes in f(R) gravity

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arxiv 1210.4696 v2 pith:37FFEXIC submitted 2012-10-17 gr-qc

S. Habib Mazharimousavi , M. Kerachian , M. Halilsoy This is my paper · ORCID
classification gr-qc
keywords blackgravityholesexistencetypeavailableconditionsderive
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We investigate the existence of Reissner-Nordstr\"om (RN) type black holes in f(R) gravity. Our emphasis is to derive, in the presence of electrostatic source, the necessary conditions which provide such static, spherically symmetric (SSS) black holes available in f(R) gravity. We also study the thermodynamics of the black hole solution.

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  1. Effective Metric Description of Charged Black Holes

    gr-qc 2025-04 conditional novelty 6.0 of 10

    Near-extremal and extremal charged black holes can be described by an effective metric built from the proper time of an infalling observer, with explicit consistency constraints on the deformation parameters.

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