Bianchi type V barotropic fluid cosmological model with bulk viscosity and time dependent displacement vector in Lyra geometry
*Department of Mathematics, University of Rajasthan Jaipur India
Email:-balir5@yahoo.co.in
Bianchi Type V bulk viscous cosmological model for barotropic fluid distribution (p = gr, 0 £ g £ 1, p being the isotropic pressure, r the matter density) with time dependent displacement vector in the frame work of Lyra geometry is investigated. To get the deterministic solution, we have also assumed zq = constant where z the coefficient of bulk viscosity and q the expansion in the model. For g = 0 (dust distribution), we get the same model as obtained by Bali and Chandnani5. The physical and geometrical aspects of the model are also discussed.
Copy the following to cite this article:
RAJ BALI* and RAJENDRA VADHWANI , "Bianchi type V barotropic fluid cosmological model with bulk viscosity and time dependent displacement vector in Lyra geometry ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 3, Page Number 653-662, 2016Copy the following to cite this URL:
RAJ BALI* and RAJENDRA VADHWANI , "Bianchi type V barotropic fluid cosmological model with bulk viscosity and time dependent displacement vector in Lyra geometry ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 3, Page Number 653-662, 2016Available from: https://www.ultrascientist.org/paper/725/
This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License
