Thermodynamics in Kaluza-Klein Universe
arXiv:1406.4457 · doi:10.1142/S0217732313500727
Abstract
This paper is devoted to check the validity of laws of thermodynamics for Kaluza-Klein universe in the state of thermal equilibrium, composed of dark matter and dark energy. The generalized holographic dark energy and generalized Ricci dark energy models are considered here. It is proved that the first and generalized second law of thermodynamics are valid on the apparent horizon for both of these models. Further, we take a horizon of radius with modified holographic or Ricci dark energy. We conclude that these models do not obey the first and generalized second law of thermodynamics on the horizon of fixed radius for a specific range of model parameters.
14 pages, 1 figure
References in corpus (11)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Cosmological Evolution of a Quintom Model of Dark Energy
- A Holographic Dark Energy Model from Ricci Scalar Curvature
- Dark Energy and Gravity
- Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
- Thermodynamics second law and crossing(s) in interacting holographic dark energy model
- Validity of the Generalized Second Law of Thermodynamics of the Universe Bounded by the Event Horizon in Holographic Dark Energy Model
- Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
- Generalized Holographic and Ricci Dark Energy Models
- Thermodynamical properties of dark energy with the equation of state