Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter

We study the Bianchi type-V string cosmological model with bulk viscosity in f(R,T) theory of gravity by considering a special form and linearly varying deceleration parameter. This is an extension of the earlier work of Naidu et al., 2013, where they have constructed the model by considering a cons...

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Main Authors: Bïnaya K. Bishi, K. L. Mahanta
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2015/491403
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author Bïnaya K. Bishi
K. L. Mahanta
author_facet Bïnaya K. Bishi
K. L. Mahanta
author_sort Bïnaya K. Bishi
collection DOAJ
description We study the Bianchi type-V string cosmological model with bulk viscosity in f(R,T) theory of gravity by considering a special form and linearly varying deceleration parameter. This is an extension of the earlier work of Naidu et al., 2013, where they have constructed the model by considering a constant deceleration parameter. Here we find that the cosmic strings do not survive in both models. In addition we study some physical and kinematical properties of both models. We observe that in one of our models these properties are identical to the model obtained by Naidu et al., 2013, and in the other model the behavior of these parameters is different.
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spelling doaj-art-372ba321a9984869823c174e037a97f42025-02-03T01:04:48ZengWileyAdvances in High Energy Physics1687-73571687-73652015-01-01201510.1155/2015/491403491403Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration ParameterBïnaya K. Bishi0K. L. Mahanta1Department of Mathematics, Visvesvaraya National Institute of Technology, Nagpur 440010, IndiaDepartment of Mathematics, C.V. Raman College of Engineering, Bidya Nagar, Mahura, Janla, Bhubaneswar 752054, IndiaWe study the Bianchi type-V string cosmological model with bulk viscosity in f(R,T) theory of gravity by considering a special form and linearly varying deceleration parameter. This is an extension of the earlier work of Naidu et al., 2013, where they have constructed the model by considering a constant deceleration parameter. Here we find that the cosmic strings do not survive in both models. In addition we study some physical and kinematical properties of both models. We observe that in one of our models these properties are identical to the model obtained by Naidu et al., 2013, and in the other model the behavior of these parameters is different.http://dx.doi.org/10.1155/2015/491403
spellingShingle Bïnaya K. Bishi
K. L. Mahanta
Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
Advances in High Energy Physics
title Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
title_full Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
title_fullStr Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
title_full_unstemmed Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
title_short Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter
title_sort bianchi type v bulk viscous cosmic string in f r t gravity with time varying deceleration parameter
url http://dx.doi.org/10.1155/2015/491403
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