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Turkish Journal of Physics

DOI

10.3906/fiz-1710-23

Abstract

Here we investigate spatially flat Friedmann-Robertson-Walker space-time models of the universe to study the thermodynamic behaviors in light of variables $G$ and $\Lambda $. A particular method to find the solutions of Einstein's field equations and mathematical expressions for temperature and entropy of the perfect fluid cosmological models is introduced by using both the equation of state and the assumption $G=G_{0} \,a^{n}$. It is observed that the phantom field of ($\omega

Keywords

Cosmology, cosmological constant, thermodynamics, singularities

First Page

198

Last Page

209

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