English

An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe

General Relativity and Quantum Cosmology 2015-05-01 v2

Abstract

We study the evolution of the dark energy parameter within the scope of a spatially flat and isotropic Friedmann-Robertson-Walker (FRW) model filled with barotropic fluid and dark energy. To obtain the deterministic solution we choose the scale factor a(t)=teta(t) = \sqrt{t e^{t}} which yields a time dependent deceleration parameter (DP). In doing so we consider the case minimally coupled with dark energy to the perfect fluid as well as direct interaction with it.

Keywords

Cite

@article{arxiv.1011.3940,
  title  = {An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe},
  author = {Hassan Amirhashchi and Anirudh Pradhan and Bijan Saha},
  journal= {arXiv preprint arXiv:1011.3940},
  year   = {2015}
}

Comments

11 pages, accepted for publication in Chinese Physics Letters. Unlike the previous version the new one contains the time depending deceleration parameter