The charged McVittie spacetime
arXiv:1404.3929 · doi:10.1103/PhysRevD.89.103514
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.
References in corpus (9)
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- Black Hole Evaporation in an Expanding Universe
- Black holes and black hole thermodynamics without event horizons
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- Charged black holes in expanding Einstein-de Sitter universes
- Evolution of black holes through a nonsingular cosmological bounce
- Dynamical model for primordial black holes
- Debye Screening of Non-Abelian Plasmas in Curved Spacetimes
- Dynamical black holes and accretion-induced backreaction
- Local coordinates and motion of a test particle in the McVittie spacetime
- Dark matter halos modeled by polytropic spheres influenced by the relict cosmological constant and trapping polytropes forming supermassive black holes
- Black-hole evaporation for cosmological observers
- Spherically symmetric solutions in a FRW background
- Masses dynamics during black hole evaporation in spatially flat FLRW universes
- New charged dynamical particles in spatially flat FLRW space-times