doi: 10.7763/IJAPM.2012.V2.131
Tilted Bulk Disordered Distribution Cosmological Model
Rakeshwar Purohit
1
,
Anita Bagora
2
- 1 M. L. Sukhadia University, Udaipur-313001, India
- 2 the Jaipur National University, Jaipur-302025, India
Abstract
Bianchi type I bulk viscous fluid tilted cosmological model filled with disordered radiation and heat conduction is investigated. We assume that <i>ζ</i>θ= K (constant), where <i>ζ </i>is the coefficient of bulk viscosity and θ is the expansion in the model. It has been assumed that the expansion in the model is only in two directions i.e. one of the component of Hubble parameter (<i>H<sub>1</sub>=A<sub>4</sub>/A</i>) is zero. The physical and geometrical aspects of the model in the presence and absence of bulk viscosity are also discussed.
Keywords
- Tilted cosmological model
- bulk viscosity
- Bianchi type-I universe
How to Cite
Rakeshwar Purohit and Anita Bagora, "Tilted Bulk Disordered Distribution Cosmological Model," International Journal of Applied Physics and Mathematics, vol. 2, no. 5, pp. 348-351, 2012. https://doi.org/ 10.7763/IJAPM.2012.V2.131
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).