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