FRW Cosmological Model in Linear f(T) Gravity Using Hybrid Expansion Law
Authors/Creators
- 1. P. G. Department of Mathematics, Yashwantrao Chavan Arts and Science Mahavidyalaya, Mangrulpir, Dist. Washim, (M.S.) India
- 2. Prof Ram Meghe College of Engineering & Management, Badnera - Amravati, (M.S.) India
- 3. Department of Mathematics, Indira Gandhi Mahavidyalaya, Ralegaon, (M.S.) India
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Description
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.
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