Bianchi Type-VIo Wet Dark Fluid Cosmological Model with Linearly Varying Deceleration Parameter in f(R,T) Gravity

Authors(3) :-A. Y. Shaikh, K. S. Wankhade, S. R. Bhoyar

In this paper, Bianchi type- VIo cosmological model with Wet Dark Fluid (WDF) in f(R,T) gravity , where R is the Ricci scalar and T the trace of stress energy-momentum tensor, in the context of late time accelerating expansion of the universe has been studied. The exact solutions of the field equations are obtained by using a linearly varying deceleration parameter (LVDP). The universe ends with big rip. Our model initially shows acceleration for a certain period of time and then decelerates consequently. Several dynamical and physical behaviors of the model are also discussed in detail.

Authors and Affiliations

A. Y. Shaikh
Department of Mathematics , Indira Gandhi Mahavidyalaya, Ralegaon, Maharashtra, India
K. S. Wankhade
Department of Mathematics , Y.C.Science College , Mangrulpir, Maharashtra, India
S. R. Bhoyar
Department of Mathematics , Phulsing Naik Mahavidyalaya Pusad, Maharashtra, India

Bianchi type VI0 space-time, f(R,T) gravity; WDF, LVDP

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Publication Details

Published in : Volume 3 | Issue 8 | November-December 2017
Date of Publication : 2017-12-31
License:  This work is licensed under a Creative Commons Attribution 4.0 International License.
Page(s) : 1248-1254
Manuscript Number : IJSRST1738186
Publisher : Technoscience Academy

Print ISSN : 2395-6011, Online ISSN : 2395-602X

Cite This Article :

A. Y. Shaikh, K. S. Wankhade, S. R. Bhoyar, " Bianchi Type-VIo Wet Dark Fluid Cosmological Model with Linearly Varying Deceleration Parameter in f(R,T) Gravity", International Journal of Scientific Research in Science and Technology(IJSRST), Print ISSN : 2395-6011, Online ISSN : 2395-602X, Volume 3, Issue 8, pp.1248-1254, November-December-2017.
Journal URL : https://ijsrst.com/IJSRST1738186
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