Emergent Universe with Interacting fluids and Generalized Second Law of Thermodynamics
arXiv:1503.08284 · doi:10.1088/0264-9381/32/11/115001
Abstract
We investigate the emergent universe scenario in the presence of interacting fluids. The non-linear equation of state (EoS) considered in the general theory of relativity for obtaining emergent universe is effectively a cosmological model with a composition of three fluids. In this paper we consider two models to realize viable cosmological scenarios, {\it viz.}, (i) a two-fluid model with interaction of a pressureless fluid with the fluid having the non-linear EoS needed for the emergent universe, and (ii) a three-fluid model with interaction among the three fluids which originate from the EoS of the emergent universe. It is found that realistic cosmological models in accordance with observations are not ruled out for both the above cases. We further show that the generalized second law of thermodynamics is found to hold good in the emergent universe with interacting fluids.
8 pages, 1 figure accepted in Classical and Quantum Gravity (2015)
References in corpus (10)
- Thermodynamic Behavior of Friedmann Equation at Apparent Horizon of FRW Universe
- Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
- Cosmologies with Energy Exchange
- Emergent Universe with Exotic Matter
- Emergent Universe and Phantom Tachyon Model
- A k-essence Model Of Inflation, Dark Matter and Dark Energy
- Emergent Universe in Brane World Scenario with Schwarzschild-de Sitter Bulk
- Cosmological Constant from the Emergent Gravity Perspective
- Interacting Cosmological Fluids and the Coincidence Problem
- An emergent universe supported by a nonlinear sigma model