Dark Energy Accretion onto a Black Hole in an Expanding Universe

Abstract

By using the solution describing a black hole embedded in the FLRW universe, we obtain the evolving equation of the black hole mass expressed in terms of the cosmological parameters. The evolving equation indicates that in the phantom dark energy universe the black hole mass becomes zero before the Big Rip is reached.

7 pages, no figures, errors is corrected

References in corpus (6)

• Dynamics of dark energy
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Cosmological expansion and local physics
• Does the mass of a black hole decrease due to the accretion of phantom energy
• Phantom Energy Accretion onto Black Holes in Cyclic Universe
• Will black holes eventually engulf the universe?

Cited by in corpus (13)

• Pilgrim Dark Energy
• Cosmological Analysis of Pilgrim Dark Energy in Loop Quantum Cosmology
• An interacting New Holographic Dark Energy in the framework of fractal cosmology
• Adiabatic accretion onto black holes in Einstein-Maxwell-scalar theory
• Cosmological Evolution of Pilgrim Dark Energy
• Black hole in a generalized Chaplygin-Jacobi dark fluid: shadow and light deflection angle
• Vacuum polarization instead of "dark matter" in a galaxy
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Fate of an Accretion Disc around a Black Hole when both the Viscosity and Dark Energy is Effecting
• Enhanced power of gravitational waves and rapid coalescence of black hole binaries through dark energy accretion
• Evolving black hole horizons in General Relativity and alternative gravity
• Embedding black holes and other inhomogeneities in the universe in various theories of gravity: a short review
• Spontaneous Symmetry Breaking Vacuum Energy in Cosmology