Entropy of cosmological black holes and generalized second law in phantom energy-dominated universe
arXiv:0907.4528 · doi:10.1142/S0218271811018743
Abstract
Adopting the thin-layer improved brick-wall method, we investigate the thermodynamics of a black hole embedded in a spatially flat Friedmann-Robertson-Walker universe. We calculate the temperature and the entropy at every apparent horizon for arbitrary solution of the scale factor. We show that the temperature and entropy display a non-trivial behavior as functions of time. In the case of black holes immersed in universe driven by phantom energy, we show that for specific ranges of the equation-of-state parameter and apparent horizons the entropy is compatible with the D-bound conjecture, even the null, dominant and strong energy conditions are violated. In the case of accretion of phantom energy onto black hole with small Hawking-Hayward quasi-local mass, we obtain an equation-of-state parameter in the range , guaranteeing the validity of the generalized second law.
20 pages, 5 figures, Major revision,Submitted to the IJMPD
References in corpus (18)
- Cosmological expansion and local physics
- Einstein's equations as a thermodynamic identity: The cases of stationary axisymmetric horizons and evolving spherically symmetric horizons
- Cosmological coincidence problem in interacting dark energy models
- Cosmic Duality in Quintom Universe
- On the Hawking radiation as tunneling for a class of dynamical black holes
- The generalized second law of thermodynamics in the accelerating universe
- 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
- Schwarzschild black hole and the generalized second law in phantom-dominated universe
- Thermodynamical properties of dark energy
- Thermodynamical properties of hairy black holes in n spacetimes dimensions
- Generalized Second Law and phantom Cosmology: accreting black holes
- Evolution of Primordial Black Holes in a radiation and phantom energy environment
- Phantom Accretion by Black Holes and the Generalized Second Law of Thermodynamics
- Entropy of the FRW cosmology based on the brick wall method
- Generalized second law in phantom dominated universe
- The Generalized Second Law in Dark Energy Dominated Universes