Evolution of a Schwarzschild Black Hole in Phantom-like Chaplygin gas Cosmologies

Abstract

In the classical relativistic regime, the accretion of phantom energy onto a black hole reduces the mass of the black hole. In this context, we have investigated the evolution of a Schwarzschild black hole in the standard model of cosmology using the phantom-like modified variable Chaplygin gas and the viscous generalized Chaplygin gas. The corresponding expressions for accretion time scale and evolution of mass have been derived. Our results indicate that mass of the black hole will decrease if the accreting phantom Chaplygin gas violates the dominant energy condition and will increase in the opposite case. Thus our results are in agreement with the results of Babichev \textit{et al} \cite{Babi1} who first proposed this scenario.

12 pages, no figures, version to appear in Eur. Phys. J. C

References in corpus (14)

• Dynamics of dark energy
• Interacting holographic generalized Chaplygin gas model
• Generalized Second Law of Thermodynamics in Quintom Dominated Universe
• Bulk Viscous Cosmology
• Charged Black Holes in Phantom Cosmology
• Interacting models of soft coincidence
• Does the mass of a black hole decrease due to the accretion of phantom energy
• Interacting Modified Variable Chaplygin Gas in Non-flat Universe
• Interacting Dark Energy with Inhomogeneous Equation of State
• WMAP5 constraints on the unified model of dark energy and dark matter
• On the formalism of dark energy accretion onto black- and worm-holes
• New "Bigs" in cosmology
• Will black holes eventually engulf the universe?
• Constraints on the unified dark energy-dark matter model from latest observational data

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