doi: 10.7763/IJAPM.2012.V2.136
Imperfect Barotropic Magnetic Tilted Cosmological Model
- 1 the Jaipur National University, Jaipur-302025, India
- 2 the M.L. Sukhadia University, Udaipur-313001, India
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=γЄ , where p being isotropic pressure, Є the matter density .It has been assumed that the expansion in the model is only in two directions i.e. one of the component of Hubble parameter is zero. Also, 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.
Keywords
- Tilted cosmological model
- magnetic field;
- bianchi type-I universe. PACS numbers: 98.80.-k
- 04.20.-q 2000 Mathematics Subject Classification: 83C50
- 83F05
How to Cite
Anita Bagora and Rakeshwar Purohit, "Imperfect Barotropic Magnetic Tilted Cosmological Model," International Journal of Applied Physics and Mathematics, vol. 2, no. 5, pp. 365-368, 2012. https://doi.org/ 10.7763/IJAPM.2012.V2.136
Copyright & License
Copyright © 2012 by the authors. This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
