The generalized second law of thermodynamics for the interacting in gravity
arXiv:1401.8283 · doi:10.1007/s10509-013-1747-0
Abstract
We study the validity of the generalized second law (GSL) of gravitational thermodynamics in a non-flat FRW universe containing the interacting in gravity. We consider that the boundary of the universe to be confined by the dynamical apparent horizon in FRW universe. In general, we discuss the effective equation of state, deceleration parameter and GLS in this framewok. Also, we find that the interacting-term modifies these quantities and in particular, the evolution of the total entropy, results in an increases on the GLS of thermodynamic, by a factor . By using a viable gravity with an exponential dependence on the torsion, we develop a model where the interaction term is related to the total energy density of matter. Here, we find that a crossing of phantom divide line is possible for the interacting- model.
16 pages and 3 figures. Astrophys.Space Sci. in press
References in corpus (17)
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- Thermodynamic Behavior of Friedmann Equation at Apparent Horizon of FRW Universe
- Friedmann Equations of FRW Universe in Scalar-tensor Gravity, f(R) Gravity and First Law of Thermodynamics
- Observational constraints on theory
- Cosmography in f(T)-gravity
- Le Chatelier-Braun principle in cosmological physics
- Thermodynamics of cosmological horizons in gravity
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Improved Constraints on the Acceleration History of the Universe and the Properties of the Dark Energy
- Interacting models of soft coincidence
- Generalized Second Law of Thermodynamics in Gravity with Entropy Corrections
- The generalized second law in phantom dominated universes in the presence of black holes
- Phase space analysis of interacting dark energy in f(T) cosmology
- Generalized second law of thermodynamics in the emergent universe for some viable models of f(T) gravity
- The generalized second law for the interacting generalized Chaplygin gas model