https://doi.org/10.1140/epjp/i2019-12583-4
Regular Article
LRS Bianchi type-I cosmological models with accelerated expansion in f(R, T) gravity in the presence of 
(T)
1
Department of Mathematics, Institute of Applied Sciences & Humanities, G L A University, 281 406, Mathura, Uttar Pradesh, India
2
Department of Mathematics, Pt. S. N. S. University, Shahdol, M. P., India
3
Department of Mathematical Sciences, University of Zululand, 3886, Kwa-Dlangezwa, South Africa
* e-mail: pradhan.anirudh@gmail.com
Received:
18
December
2017
Accepted:
19
February
2019
Published online:
27
May
2019
This paper examines the physical behaviour of the transition of the LRS Bianchi type-I perfect-fluid cosmological models from early decelerating to the current accelerating phase within the framework of the f(R,T) theory of gravity. To determine the solution of the field equations, the concept of a time-dependent deceleration parameter is used. This yields scale factors for which the universe attains a phase transition scenario, and is consistent with recent cosmological observations. Two cases are considered, firstly 
, where n and 
are positive constants. For 
, this generates a class of accelerating models, while for 
, the universe attains a phase transition from an early decelerating to the present accelerating phase. This model 1 starts from quintessence (
) initially and ended up with phantom phase 
when 
. The second case is 
, where n and k are positive constants. It is observed that for 
and 
, a class of transit models of the universe are obtained. The model 2 belongs to the scenario of phantom energy (
). We have observed the existence of type-III singularity in our model 2. Some physical and geometric properties of the models are found and discussed.
© Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature, 2019
