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

被引:73
作者
Amirhashchi, Hassan [2 ]
Pradhan, Anirudh [1 ,3 ]
Saha, Bijan [3 ]
机构
[1] Hindu Postgrad Coll, Dept Math, Zamania 232331, Ghazipur, India
[2] Islamic Azad Univ, Dept Phys, Mahshahr Branch, Mahshahr, India
[3] Joint Inst Nucl Res, Informat Technol Lab, Dubna 141980, Russia
关键词
PROBE WMAP OBSERVATIONS; HUBBLE-SPACE-TELESCOPE; ACCELERATING UNIVERSE; MATTER INTERACTION; ANISOTROPY; DECELERATION; CONSTRAINTS; SUPERNOVAE; VIOLATION; PRINCIPLE;
D O I
10.1088/0256-307X/28/3/039801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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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