4.5 Article

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

Journal

CHINESE PHYSICS LETTERS
Volume 28, Issue 3, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0256-307X/28/3/039801

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Funding

  1. Laboratory of Information Technologies, Joint Institute for Nuclear Research, Dubna, Russia

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We study the evolution of the dark energy parameter within the scope of a spatially homogeneous 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) = root te(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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