
Abstract: In the current work, we have studied spatially homogenous and isotropic flat Friedman-Robertson-Walker (FRW) cosmological model filled with perfect fluid within the context of gravity, in particular - linear model of gravity, viz. . To obtain the exact solution of the field equations, we have taken into consideration the hybrid expansion law of scale factor . We examined a few of the model's physical parameters, including energy density, pressure, equation of state (EoS) parameter, and squared sound velocity. Additionally, some of the model's kinematical properties have been discussed.
Keywords: gravity, FRW metric, Hybrid expansion law, Perfect Fluid, Cosmology., Keywords: gravity, FRW metric, Hybrid expansion law, Perfect Fluid, Cosmology.
Keywords: gravity, FRW metric, Hybrid expansion law, Perfect Fluid, Cosmology., Keywords: gravity, FRW metric, Hybrid expansion law, Perfect Fluid, Cosmology.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
