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The charged McVittie spacetime

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arxiv 1404.3929 v1 pith:VKD2IABN submitted 2014-04-15 gr-qc

Valerio Faraoni , Andres F. Zambrano Moreno , Angus Prain This is my paper · ORCID
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keywords chargedmcvittiespacetimeaccordinganalyticallyapparentblackcase
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The two-parameter charged McVittie solution of the Einstein equations is revisited and its apparent horizons are discussed and located numerically (for the extremal case, analytically). According to the parameter values, this spacetime can be interpreted as a black hole, or a spacelike naked singularity, in a spatially homogeneous and isotropic universe.

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  1. Dynamical black holes and accretion-induced backreaction

    gr-qc 2025-07 conditional novelty 4.0 of 10

    For accreting Reissner-Nordstrom black holes, the momentum flux from infalling matter splits an extremal horizon into two, while energy density displaces the extremal horizon's radius.

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