Magnetized Bianchi Type-VIo String Cosmological Model for Anti-Stiff Fluid in General Relativity

AUTHOR AND
AFFILIATION

Dhirendra Chhajed1, Ankita Choudhary*1, Atul Tyagi1

1Department of Mathematics & Statistics, University college of science,

Mohanlal Sukhadia University, Udaipur, 313001, Rajasthan, India

Corresponding author email:  ankitamaths1993@gmail.com

KEYWORDS:

Bianchi type-VI0, Anti-stiff fluid, Magnetic field, Cosmology (85A40).

Issue Date:

July-2022

Pages:

51-60

ISSN:

2319-8044 (Online) – 2231-346X (Print)

Source:

Vol.34 – No.4

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DOI:

http://dx.doi.org/10.22147/jusps-A/340401

ABSTRACT:

In this paper, we have investigated magnetized Bianchi type-VI0 string cosmological model for anti-stiff fluid in general relativity. We assume that F23 is the only survival component of electromagnetic field tensor Fij. For the absolute determination of the model, we assume the expansion in the model is proportional to the shear. The common measures of the Einstein’s field equations for the cosmological model have been acquired under the assumption of anti-stiff fluid i.e. p + ρ = 0, where ρ and p are the rest energy density and the pressure of the fluid, respectively. The physical and geometrical outcomes of the model in the presence of magnetic field are discussed.

Copy the following to cite this Article:

Dhirendra Chhajed, Ankita Choudhary, Atul Tyagi; “Magnetized Bianchi Type-Vi0 String Cosmological Model For Anti-Stiff Fluid In General Relativity”, Journal of Ultra Scientist of Physical Sciences, Volume 34, Issue 4, Page Number 51-60, March 2022


Copy the following to cite this URL:

Dhirendra Chhajed, Ankita Choudhary, Atul Tyagi; “Magnetized Bianchi Type-Vi0 String Cosmological Model For Anti-Stiff Fluid In General Relativity”, Journal of Ultra Scientist of Physical Sciences, Volume 34, Issue 4, Page Number 51-60, March 2022