Magnetized strange quark model with Big Rip singularity in f (R, T) gravity

Sahoo P. K. , Sahoo P., Bishi B. K. , Aygun S.

MODERN PHYSICS LETTERS A, vol.32, no.21, 2017 (Peer-Reviewed Journal) identifier identifier

  • Publication Type: Article / Article
  • Volume: 32 Issue: 21
  • Publication Date: 2017
  • Doi Number: 10.1142/s021773231750105x
  • Journal Indexes: Science Citation Index Expanded, Scopus
  • Keywords: LRS Bianchi type-I spacetime, linearly varying deceleration parameter, magnetized, strange quark matter, Big Rip singularity, f (R, T) gravity, BIANCHI TYPE-I, SYMMETRIC COSMOLOGICAL MODEL, STRING CLOUD, DYNAMICAL MODEL, DOMAIN-WALLS, DARK ENERGY, MATTER, F(R, UNIVERSE, FIELDS


Locally rotationally symmetric (LRS) Bianchi type-I magnetized strange quark matter (SQM) cosmological model has been studied based on f(R, T) gravity. The exact solutions of the field equations are derived with linearly time varying deceleration parameter, which is consistent with observational data (from SNIa, BAO and CMB) of standard cosmology. It is observed that the model begins with big bang and ends with a Big Rip. The transition of the deceleration parameter from decelerating phase to accelerating phase with respect to redshift obtained in our model fits with the recent observational data obtained by Farook et al. [Astrophys. T. 835, 26 (2017)]. The well-known Hubble parameter H(z) and distance modulus it(z) are discussed with redshift.