Tilted Cosmological Model With Electromagnetic Field

AUTHOR AND
AFFILIATION

ANITA BAGORA (MENARIA)

KEYWORDS:

Tilted cosmological model; Magnetic field; Bianchi type-I universe.

Issue Date:

April 2013

Pages:

ISSN:

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

Source:

Vol.25 – No.1

PDF

Click Here Download PDF

DOI:

jusps-A

ABSTRACT:

Tilted Bianchi type I cosmological model in the presence of magnetic field and barotropic fluid is investigated. To determine complete solution, we have assumed that the condition p  , where p being isotropic pressure,  the matter density and also assumed that the relation between metric potential as A=BC. Here, we have seen that Maxwell’s equations F [ij;k] = 0 is satisfied by F 23 = constant. The physical and geometrical aspects of the model in the presence and absence of magnetic field together with singularity in the model are also discussed.

Copy the following to cite this Article:

ANITA BAGORA (MENARIA), “Tilted Cosmological Model With Electromagnetic Field”, Journal of Ultra Scientist of Physical Sciences, Volume 25, Issue 1, Page Number , 2016


Copy the following to cite this URL:

ANITA BAGORA (MENARIA), “Tilted Cosmological Model With Electromagnetic Field”, Journal of Ultra Scientist of Physical Sciences, Volume 25, Issue 1, Page Number , 2016

Available from: http://www.ultrascientist.org/paper/263/


Tilted Bianchi type I cosmological model in the presence of magnetic field and barotropic fluid is investigated. To determine complete solution, we have assumed that the condition p  , where p being isotropic pressure,  the matter density and also assumed that the relation between metric potential as A=BC. Here, we have seen that Maxwell’s equations F [ij;k] = 0 is satisfied by F 23 = constant. The physical and geometrical aspects of the model in the presence and absence of magnetic field together with singularity in the model are also discussed.