What is the fate of a black hole embedded in an expanding universe?
arXiv:0811.4667 · doi:10.1016/j.physletb.2008.11.067
Abstract
Within a large class of exact solutions of the Einstein equations describing a black hole embedded in a Friedmann universe it is shown that, under certain assumptions, only those with comoving Hawking-Hayward quasi-local mass are generic, in the sense that they are late-time attractors.
9 pages, LaTex, to appear in Phys. Lett. B
References in corpus (10)
- Cosmological expansion and local physics
- Einstein's equations as a thermodynamic identity: The cases of stationary axisymmetric horizons and evolving spherically symmetric horizons
- On the Hawking radiation as tunneling for a class of dynamical black holes
- Does the mass of a black hole decrease due to the accretion of phantom energy
- The generalized second law in phantom dominated universes in the presence of black holes
- Black Hole Evaporation in an Expanding Universe
- Dynamical black holes with symmetry in Einstein-Gauss-Bonnet gravity
- The Hawking temperature of expanding cosmological black holes
- Evolution of Primordial Black Holes in a radiation and phantom energy environment
- Global structure and physical interpretation of the Fonarev solution for a scalar field with exponential potential
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- Horndeski meets McVittie: A scalar field theory for accretion onto cosmological black holes
- Dynamical apparent horizons in inhomogeneous Brans-Dicke universes
- Black holes in realistic branes: black string-like objects?
- Charged black holes in expanding Einstein-de Sitter universes
- Dynamical model for primordial black holes
- Can an evolving Universe host a static event horizon?