Magnetized strange quark matter in reconstructed f(R, T) gravity for Bianchi I and V universes with cosmological constant


TURKISH JOURNAL OF PHYSICS, vol.41, no.5, pp.469-476, 2017 (ESCI) identifier identifier

  • Publication Type: Article / Article
  • Volume: 41 Issue: 5
  • Publication Date: 2017
  • Doi Number: 10.3906/fiz-1706-4
  • Journal Indexes: Emerging Sources Citation Index (ESCI), Scopus, TR DİZİN (ULAKBİM)
  • Page Numbers: pp.469-476
  • Keywords: f(R,T) gravity, Bianchi I universe, Bianchi V universe, magnetized strange quark, deceleration parameter
  • Çanakkale Onsekiz Mart University Affiliated: Yes


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) = alpha R-1+alpha(2)f(3)(T) gravity (here alpha(1) and alpha(2) are constants; f(3) (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 ->infinity, we get the dark energy model (p = -rho) in reconstructed f (R, T) = alpha R-1 + alpha(2)f(3)(T) gravity. However, we obtain zero magnetic field in all f (R,T) gravitation models.