The Study of Consumers' impulse buying behaviour

Abstract

Abstract: We have examined the spatially homogenous and anisotropic Bianchi type-III cosmological model in the context of f(T) gravity, with the presence of holographic dark energy. Our work of a cosmological model contains a suitable function action, f(T). A straight forward power-law form of a metric potential is used to solve field equations by utilizing the relationship between the metric potentials A = tn. The primary objective of this paper is to investigate certain physically relevant concerns about the universe's evolution. It is noted that the anisotropic parameter Am is constant and that the Hubble parameter (H) , scalar expansion (θ), and shear scalar (σ) diverge at the beginning era as they get nearly to zero for high values of time. The universe is currently accelerating, as shown by the negative value of deceleration parameters.