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• W2011303350 abstract "Einstein's field equations with variable gravitational and cosmological constants are considered in the presence of perfect fluid for a spatially homogeneous and isotropic universe. Exact solutions of the field equations are obtained by using the gamma-law equation of state p=(γ-1)ρ, where the adiabatic parameter γ, varies with cosmic time. The functional form of γ, which is assumed to be the function of scale factor R as proposed by Carvalho, is used to describe the early evolution of universe. A unified description of early universe is given in which an inflationary phase is followed by radiation-dominated phase. The various physical aspects of the models are also discussed." @default.
• W2011303350 created "2016-06-24" @default.
• W2011303350 creator A5052235033 @default.
• W2011303350 date "2006-07-30" @default.
• W2011303350 modified "2023-10-16" @default.
• W2011303350 title "UNIFIED DESCRIPTION OF EARLY UNIVERSE WITH VARIABLE GRAVITATIONAL AND COSMOLOGICAL CONSTANTS" @default.
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• W2011303350 doi "https://doi.org/10.1142/s0217732306020433" @default.
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