Bianchi types I and V bulk viscous fluid cosmological models in f(R, T ) gravity theory

Ram, Shri; Kumari, Priyanka

dc.contributor.author	Ram, Shri
dc.contributor.author	Kumari, Priyanka
dc.date.accessioned	2020-03-16T10:30:26Z
dc.date.available	2020-03-16T10:30:26Z
dc.date.issued	2014-05-20
dc.identifier.issn	18951082
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/765
dc.description.abstract	In this paper we present non-singular Bianchi types I and V cosmological models, in the presence of bulk viscous fluid and within the framework of f(R,T) gravity theory. Exact solutions to the field equations are obtained by choosing a particular form of the function f(R,T) and a special value for the average scale factor of the model, which corresponds to a time- dependent deceleration parameter. The cosmological models initially accelerate for a certain period of time and thereafter decelerate. The physical and kinematical properties of the models of the universe are discussed.	en_US
dc.description.sponsorship	The authors are extremely grateful to the anonymous referees for their valuable suggestions to improve the quality of the papers. One of the authors, Priyanka Kumari, is thankful to Indian Institute of Technology (Banaras Hindu University) Varanasi for financial support.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Versita	en_US
dc.subject	Bianchi types I and V	en_US
dc.subject	Bulk viscous fluid	en_US
dc.subject	f(R, T) gravity	en_US
dc.title	Bianchi types I and V bulk viscous fluid cosmological models in f(R, T ) gravity theory	en_US
dc.type	Article	en_US