Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity

This paper deals with the bulk viscous Bianchi type-V cosmological model with an exponential scale factor in Lyra geometry based on f(R, T) gravity, by considering a time dependent displacement field. To determine the nature and physical properties of the model, we considered Harko et al. (Harko et...

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Main Authors: Bishnu Prasad Brahma, Mukunda Dewri
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-02-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.831431/full
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author Bishnu Prasad Brahma
Mukunda Dewri
author_facet Bishnu Prasad Brahma
Mukunda Dewri
author_sort Bishnu Prasad Brahma
collection DOAJ
description This paper deals with the bulk viscous Bianchi type-V cosmological model with an exponential scale factor in Lyra geometry based on f(R, T) gravity, by considering a time dependent displacement field. To determine the nature and physical properties of the model, we considered Harko et al. (Harko et al., Phys. Rev. D, 2011, 84, 024020) [proposed the linear form f(R, T) = f1(R) + f2(T)], in which the barotropic equation of state for pressure, density, and bulk viscous pressure is proportional to energy density. The kinematical properties of the model are also discussed in the presence of bulk viscosity. Evolution of energy conditions is also studied and examined the behaviour of that in examined in order to explain the late-time cosmic acceleration.
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spelling doaj.art-dee9ac3cab9845bc82298ff7cf6e45972022-12-21T17:23:59ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2022-02-01910.3389/fspas.2022.831431831431Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of GravityBishnu Prasad BrahmaMukunda DewriThis paper deals with the bulk viscous Bianchi type-V cosmological model with an exponential scale factor in Lyra geometry based on f(R, T) gravity, by considering a time dependent displacement field. To determine the nature and physical properties of the model, we considered Harko et al. (Harko et al., Phys. Rev. D, 2011, 84, 024020) [proposed the linear form f(R, T) = f1(R) + f2(T)], in which the barotropic equation of state for pressure, density, and bulk viscous pressure is proportional to energy density. The kinematical properties of the model are also discussed in the presence of bulk viscosity. Evolution of energy conditions is also studied and examined the behaviour of that in examined in order to explain the late-time cosmic acceleration.https://www.frontiersin.org/articles/10.3389/fspas.2022.831431/fullbianchi type-Vlyra geometrybulk viscousdark energyΛ CDM modelf(R, T) gravity
spellingShingle Bishnu Prasad Brahma
Mukunda Dewri
Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
Frontiers in Astronomy and Space Sciences
bianchi type-V
lyra geometry
bulk viscous
dark energy
Λ CDM model
f(R, T) gravity
title Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
title_full Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
title_fullStr Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
title_full_unstemmed Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
title_short Bulk Viscous Bianchi Type-V Cosmological Model in f(R, T) Theory of Gravity
title_sort bulk viscous bianchi type v cosmological model in f r t theory of gravity
topic bianchi type-V
lyra geometry
bulk viscous
dark energy
Λ CDM model
f(R, T) gravity
url https://www.frontiersin.org/articles/10.3389/fspas.2022.831431/full
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