Magnetized strange quark matter in reconstructed f(R, T) gravity for Bianchi I and V universes with cosmological constant
Yükleniyor...
Dosyalar
Tarih
2017
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Tubitak Scientific & Technological Research Council Turkey
Erişim Hakkı
info:eu-repo/semantics/openAccess
Özet
In this article, we have investigated the behaviors of magnetized strange quark matter distributions for Bianchi I and V universes in reconstructed f (R, T) = α1R+α2f3(T) gravity (here α1 and α2 are constants; f3(T) is an arbitrary function of T). To get solutions of the field equations we have used a deceleration parameter and the equation of state for strange quark matter. The new represented f(R,T) model includes two models of Harko et al. and transforms to general relativity. When t → ∞, we get the dark energy model (p = −ρ) in reconstructed f (R, T) = α1R + α2f3(T) gravity. However, we obtain zero magnetic field in all f(R, T) gravitation models.
Açıklama
Anahtar Kelimeler
f(R,T) gravity, Bianchi I universe, Bianchi V universe, magnetized strange quark, deceleration parameter
Kaynak
Turkish Journal of Physics
WoS Q Değeri
N/A
Scopus Q Değeri
Q2
Cilt
41
Sayı
5
