Axially magnetized Dark Energy cosmological model

Abstract

We investigate the behaviour of the skewness parameters for an anisotropic universe in the framework of General Relativity. Non interacting dark energy is considered in presence of electromagnetic field. A time varying deceleration parameter simulated by a hybrid scale factor is considered. The dynamics of the universe is investigated in presence and absence of magnetic field. The equation of state parameter of dark energy evolves within the range predicted by the observations. Magnetic field is observed to have a substantial effect on the cosmic dynamics and the skewness parameters. The models discussed here end in a big rip and become isotropic at finite time.

9 pages, 13 figures, Version accepted for publication in Mod. Phys. Lett. A

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Cited by in corpus (7)

• Model parameters in the context of late time cosmic acceleration in $f(Q,T)$ gravity
• Cosmological models with a Hybrid Scale Factor
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Accelerating models with a hybrid scale factor in extended gravity
• Stability analysis of two-fluid dark energy models
• Generalized Interacting Dark Energy Model and Loop Quantum Cosmology
• An exact solution of the observable universe in Bianchi V space-time