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


AKTAŞ C.

TURKISH JOURNAL OF PHYSICS, cilt.41, ss.469-476, 2017 (ESCI İndekslerine Giren Dergi) identifier identifier

  • Cilt numarası: 41 Konu: 5
  • Basım Tarihi: 2017
  • Doi Numarası: 10.3906/fiz-1706-4
  • Dergi Adı: TURKISH JOURNAL OF PHYSICS
  • Sayfa Sayıları: ss.469-476

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) = 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.