Dynamics of Bianchi cosmological model in Rn gravity

The LRS Bianchi-I spatially homogeneous and anisotropic perfect fluid cosmological model is studied in f(R,T) theory by specific choice of f(R,T)=R+αRn+λT. In this paper, to get the deceleration parameter as a function of time (t), the scale factor is considered as an increasing function of time. By...

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Bibliographic Details
Main Authors: T. Vinutha, K. Sri Kavya
Format: Article
Language:English
Published: Elsevier 2021-04-01
Series:Results in Physics
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S2211379721000462