Magnetized strange quark model with Big Rip singularity in gravity
arXiv:1703.08430 · doi:10.1142/S021773231750105X
Abstract
LRS (Locally Rotationally symmetric) Bianchi type-I magnetized strange quark matter cosmological model have been studied based on 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 start with big bang and ends with a Big Rip. The transition of 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. in 2017. The well known Hubble parameter and distance modulus are discussed with redshift.
Accepted for publication in MPLA
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Cited by in corpus (13)
- Bouncing cosmological solutions from f(R,T) gravity
- Construction of Charged Cylindrical Gravastar-like Structures
- A periodic varying deceleration parameter in gravity
- LRS Bianchi type-I cosmological model with constant deceleration parameter in gravity
- Magnetized strange quark matter in gravity with bilinear and special form of time varying deceleration parameter
- gravity models as alternatives to cosmic acceleration
- Viability of Bianchi type V Universe in gravity
- FLRW cosmological models with quark and strange quark matters in f(R,T) gravity
- Invariant Bianchi type I models in Gravity
- Dynamical Instability of Spherical Anisotropic Sources in Gravity
- Phantom energy dominated universe as a transient stage in cosmology
- Mixed fluid cosmological model in gravity
- Metric-Affine Myrzakulov Gravity Theories