Year: 2022
Type: article
Abstract: The spatially homogeneous and fully anisotropic LRS Bianchi Type-II space-time dark energy model with the EOS parameter is taken into account in the context of Harko et al. f(R, T) gravity (Phys. Rev. D, 84:024020, 2011). A dark energy cosmological model is generated in this theory using Berman's (Nuovo Cimento B, 74:182, 1983) unique law of variation for Hubble's parameter. With the proper selection of a function, we examine the modification R, f (T) in Bianchi type-II cosmology using the f(R,T) model. To obtain the solution, we use the power law relationship between the average Hubble parameter H and the average scale factor R. The power law model and the exponential model are the two universe models that result from the assumption of a constant deceleration parameter. The model's physical and kinematical characteristics are also explored.
Author: Ghanshyam Sen , Sudha Agrawal
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W7218565801