Thermodynamical description of interacting entropy-corrected new agegraphic dark energy
arXiv:1007.3985 · doi:10.1209/0295-5075/93/69001
Abstract
To explain the accelerating universe driven by dark energy, a so-called "entropy-corrected new agegraphic dark energy" (ECNADE), was recently proposed with the help of quantum corrections to the entropy-area relation in the framework of loop quantum cosmology. Using this definition, we study its thermodynamical features including entropy and energy conservation. We discuss the thermodynamical interpretation of the interaction between ECNADE and dark matter in a non-flat universe bounded by the apparent horizon. We obtain a relation between the interaction term of the dark components and thermal fluctuation.
8 pages, version accepted for publication in Europhysics Letters (2011)
References in corpus (25)
- A Dark Energy Model Characterized by the Age of the Universe
- A New Model of Agegraphic Dark Energy
- Hawking Radiation of Apparent Horizon in a FRW Universe
- Quantum Tunneling and Back Reaction
- Noncommutative Black Hole Thermodynamics
- Cosmological Constraints on New Agegraphic Dark Energy
- Instability of agegraphic dark energy models
- Black hole quantum tunnelling and black hole entropy correction
- Fermion Tunneling Beyond Semiclassical Approximation
- Interacting Agegraphic Dark Energy
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Quantum Tunneling and Trace Anomaly
- Corrected entropy of BTZ black hole in tunneling approach
- Agegraphic dark energy as a quintessence
- Interacting agegraphic dark energy models in non-flat universe
- Quintessence reconstruction of the new agegraphic dark energy model
- Exact Differential and Corrected Area Law for Stationary Black Holes in Tunneling Method
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- Interacting Modified Variable Chaplygin Gas in Non-flat Universe
- New agegraphic dark energy model with generalized uncertainty principle
- Constraints on coupling constant between dark energy and dark matter
- Interacting Dark Energy with Inhomogeneous Equation of State
- Origin of holographic dark energy models
- Agegraphic Chaplygin gas model of dark energy
- Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe