arXiv · 1011.3940
An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
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 $a(t) = \sqrt{t e^{t}}$ 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.
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Hassan Amirhashchi, Anirudh Pradhan, Bijan Saha. 2011-01-14. An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe. https://doi.org/10.1088/0256-307x%2F28%2F3%2F039801
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