Black Holes in Accelerated Universe

Abstract

We have analyzed the evolution of mass of a stationary black hole in the standard FRW cosmological model. The evolution is determined specifically about the time of transition from the earlier matter to the later exotic dark energy dominated universe. It turns out that the accretion rate of matter on the black hole of mass $M$ was approximately $10^{54}{M}^{-1}$ higher than the accretion rate of exotic dark energy at the time of transition.

8 pages

References in corpus (14)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
• Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models
• Interacting Holographic Phantom
• Cosmic Duality in Quintom Universe
• Charged Black Holes in Phantom Cosmology
• A String-Inspired Quintom Model Of Dark Energy
• Interacting Modified Variable Chaplygin Gas in Non-flat Universe
• Comparison of Approaches to Quantum Correction of Black Hole Thermodynamics
• Interacting Dark Energy with Inhomogeneous Equation of State
• Crossing of the w=-1 Barrier in Two-Fluid Viscous Modified Gravity
• On the Eddington limit in accretion discs
• Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
• Phantom dark energy and cosmological solutions without the Big Bang singularity

Cited by in corpus (5)

• Resolution of dark matter problem in f(T) gravity
• Generalized Second Law of Thermodynamics for FRW Cosmology with Power-Law Entropy Correction
• Evolution of Primordial Black Holes in Loop Quantum Gravity
• Generalized Interacting Dark Energy Model and Loop Quantum Cosmology
• Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies