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Axially magnetized dark energy cosmological model

B. Mishra

Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, India

E-mail Address: bivudutta@yahoo.com

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Pratik P. Ray

Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, India

E-mail Address: pratik.chika9876@gmail.com

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S. K. Tripathy

http://orcid.org/0000-0001-5154-2297

Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

E-mail Address: tripathy_sunil@rediffmail.com

Corresponding author.

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, and

Kazuharu Bamba

Division of Human Support System, Faculty of Symbiotic Systems Science, Fukushima University, Fukushima 960-1296, Japan

E-mail Address: bamba@sss.fukushima-u.ac.jp

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https://doi.org/10.1142/S0217732319502171Cited by:13 (Source: Crossref)

Abstract

We investigate the behavior 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.

Keywords:

PACS: 04.50.kd

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