Archives of Current Research International, ISSN: 2454-7077,Vol.: 11, Issue.: 2

Original-research-article

The Behaviour of Magnetized Strange Quark Matter on Bianchi V I_h Universe in the Framework of f(R,T) Theory

Sezgin Aygün^1*, Can Aktaş² and İhsan Yılmaz^3
1Department of Physics, Çanakkale Onsekiz Mart University, Arts and Sciences Faculty, Terzioğlu Campus, 17020, Turkey.
²Department of Mathematics, Çanakkale Onsekiz Mart University, Arts and Sciences Faculty, Terzioğlu Campus, 17020, Turkey.
³Department of Computer Engineering, Çanakkale Onsekiz Mart University, Engineering Faculty, Terzioğlu Campus, 17020, Turkey.

Article Information
Editor(s):
(1) Sahaj Gandhi, Prof., Dept. of Physics, BhavanS College, Sardar Patel Univ., India.
(2) Sivakumar Manickam, Professor, Chemical and Nanopharmaceutical Process Engineering, Associate Dean, Research and Knowledge Exchange, Nanotechnology and Advanced Materials (NATAM), The University of Nottingham Malaysia Campus, Malaysia.
Reviewers:
(1) Vitalii Okorokov, National Research Nuclear Univ., Moscow Engineering Physics Institute, Russia.
(2) Francisco Bulnes, Technological Institute of High Studies of Chalco, Mexico.
(3) Choong-Gun Sim, University of Chungbuk Health Science, South Korea.
(4) Taxiarchis Papakostas, Technological Educational Institute of Crete, Greece.
(5) Anonymous Reviewer, University of Cape Town, South Africa.
Complete Peer review History: http://www.sciencedomain.org/review-history/22336

In this paper we have investigated Bianchi V I_h universe model with magnetized strange quark matter (MSQM) distribution in f (R,T) gravity. For the solutions of modified field equations we have used the EoS of strange quark matter and anisotropy parameter with α = 1,-1,0 in Bianchi V I_h universe. We get magnetic field for α = -1 parameter but we obtain h² = 0 for α = 1 and α = 0 parameters in Bianchi V I_h models. At the end of time, we get dark energy model for α = 1 and α = 0 models i.e. we get ρ = -p = B_c. We conclude that the source of cosmological !term may be SQM i.e. the source of dark energy may be SQM. These results agree with the solutions of Aktaş and Aygün also Aygün et al. in f (R,T) theory. Also, we get magnetized strange quark matter distribution in Einstein’s general relativity theory with ∧ for this model.

Keywords :

Strange quark matter; bianchi V I_h; f(R,T) theory; magnetic field.

Full Article - PDF    Page 1-8

DOI : 10.9734/ACRI/2017/37868