Aygün, Sezgin and Aktaş, Can and Yılmaz, İhsan (2017) The Behaviour of Magnetized Strange Quark Matter on Bianchi V Ih Universe in the Framework of f(R,T) Theory. Archives of Current Research International, 11 (2). pp. 1-8. ISSN 24547077
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Abstract
In this paper we have investigated Bianchi V Ih 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 Ih universe. We get magnetic field for α = -1 parameter but we obtain h2 = 0 for α = 1 and α = 0 parameters in Bianchi V Ih models. At the end of time, we get dark energy model for α = 1 and α = 0 models i.e. we get ρ = -p = Bc. 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.
Item Type: | Article |
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Subjects: | STM Digital Press > Multidisciplinary |
Depositing User: | Unnamed user with email support@stmdigipress.com |
Date Deposited: | 06 May 2023 09:29 |
Last Modified: | 13 Sep 2024 07:42 |
URI: | http://publications.articalerewriter.com/id/eprint/753 |