Charged McVittie spacetime
Valerio FaraoniPhysics Department and STAR Research Cluster, Bishop’s University Sherbrooke, Québec, Canada J1M 1Z7Andres F. Zambrano MorenoPhysics Department and STAR Research Cluster, Bishop’s University Sherbrooke, Québec, Canada J1M 1Z7Angus PrainPhysics Department and STAR Research Cluster, Bishop’s University Sherbrooke, Québec, Canada J1M 1Z7
2014en
ABI
Abstract
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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