According to Babichev et al., the accretion of a phantom test fluid onto a Schwarzschild black hole will induce the mass of the black hole to decrease, however the backreaction was ignored in their calculation. Using new exact solutions describing black holes in a background Friedmann-Robertson-Walker universe, we find that the physical black hole mass may instead increase due to the accretion of phantom energy. If this is the case, and the future universe is dominated by phantom dark energy, the black hole apparent horizon and the cosmic apparent horizon will eventually coincide and, after that, the black hole singularity will become naked in finite comoving time before the big rip occurs, violating the cosmic censorship conjecture
We study the evolution of primordial black holes (PBHs) in an adiabatic FLRW universe with dissipati...
AbstractThe Babichev–Dokuchaev–Eroshenko model for the accretion of dark energy onto black holes has...
Abstract- Throughout the cosmic evolution currently believed cosmic ‘critical density ’ can be shown...
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an ...
AbstractBabichev, Dokuchaev and Eroshenko have recently found that accretion of phantom energy onto ...
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an ...
We conjecture that black holes, whether accreting matter or not, can also lose mass to phantom energ...
We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Sc...
In this work we extend previous work on the evolution of a primordial black hole (PBH) to address th...
The SNe type Ia data admit that the universe today may be dominated by some exotic matter with negat...
In this work, we study the evolution of primordial black holes within the context of Brans–Dicke the...
As it follows from the classical analysis, the typical final state of a dark energy universe where a...
The SNe type Ia data admit that the Universe today may be dominated by some exotic matter with negat...
Black Holes cause a ‘pressure’ difference when consuming mass, causing Universal expansion and dark ...
Primordial black holes (PBHs) lose mass by Hawking evaporation. For sufficiently small PBHs, they ma...
We study the evolution of primordial black holes (PBHs) in an adiabatic FLRW universe with dissipati...
AbstractThe Babichev–Dokuchaev–Eroshenko model for the accretion of dark energy onto black holes has...
Abstract- Throughout the cosmic evolution currently believed cosmic ‘critical density ’ can be shown...
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an ...
AbstractBabichev, Dokuchaev and Eroshenko have recently found that accretion of phantom energy onto ...
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an ...
We conjecture that black holes, whether accreting matter or not, can also lose mass to phantom energ...
We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Sc...
In this work we extend previous work on the evolution of a primordial black hole (PBH) to address th...
The SNe type Ia data admit that the universe today may be dominated by some exotic matter with negat...
In this work, we study the evolution of primordial black holes within the context of Brans–Dicke the...
As it follows from the classical analysis, the typical final state of a dark energy universe where a...
The SNe type Ia data admit that the Universe today may be dominated by some exotic matter with negat...
Black Holes cause a ‘pressure’ difference when consuming mass, causing Universal expansion and dark ...
Primordial black holes (PBHs) lose mass by Hawking evaporation. For sufficiently small PBHs, they ma...
We study the evolution of primordial black holes (PBHs) in an adiabatic FLRW universe with dissipati...
AbstractThe Babichev–Dokuchaev–Eroshenko model for the accretion of dark energy onto black holes has...
Abstract- Throughout the cosmic evolution currently believed cosmic ‘critical density ’ can be shown...