K.S. Chandan, A. Ameen & R. P.Wankhade
In this investigation we discussed the performance between Equation of State parameter (EoS) parameter for an ideal fluid and Hydrodynamic fluid with some consequences of FRW model. According to the recent observations of SNe-Ia supernova indicate that the expansion of the universe is accelerating due to an unknown form of energy which has large negative pressure known as Dark Energy. The dark energy is characterized by an Equation of State parameter where and are the pressure and energy density of an ideal fluid.
FRW model, Hydrodynamic, EoS parameter.
Please cite this article as:
K. S. Chandan, A. Ameen, R. P.Wankhade (2020). Dominations of Hydrodynamic Model Based on an Ideal Fluid for Flat FRW Model. International Journal of Recent Research and Applied Studies, 7, 7(2), 4-6.