Thermodynamics of Phantom Energy Accreting onto a Black Hole in Einstein-Power-Maxwell Gravity
arXiv:1309.0807 · doi:10.1088/0256-307X/30/10/100403
Abstract
In this paper, we investigate the phantom energy accretion onto 3D black hole formulated in Einstein-Power-Maxwell theory. We have presented the conditions for critical accretion of phantom energy onto black hole. Further, we discuss the thermodynamics of phantom energy accreting onto black hole and found that first law of thermodynamics is easily satisfied while second law and generalized second law of thermodynamics remain invalid and conditionally valid, respectively. The results for BTZ black hole can be recovered by taking Maxwellian contribution equal to zero.
10 pages, no figure, accepted for publication in Chin. Phys. Lett
References in corpus (13)
- Higher-dimensional black holes with a conformally invariant Maxwell source
- Higher-dimensional charged black holes solutions with a nonlinear electrodynamics source
- Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
- Correspondence between Holographic and Gauss-Bonnet dark energy models
- Charged Black Holes in Phantom Cosmology
- Braneworld models with a non-minimally coupled phantom bulk field: a simple way to obtain the -1-crossing at late times
- Phantom Accretion by Five Dimensional Charged Black Hole
- Dynamics of Non-adiabatic Charged Cylindrical Gravitational Collapse
- Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
- Phantom Energy Accretion by Stringy Charged Black Hole
- Dynamics of Shearfree Dissipative Collapse in f(G) Gravity
- Phantom Accretion onto the Schwarzschild de-Sitter Black Hole
- Singularities of Noncompact Charged Objects