Stability of viscous fluid in Bianchi type-VI model with cosmological constant
General Relativity and Quantum Cosmology
2013-08-29 v1 Cosmology and Nongalactic Astrophysics
Abstract
In this paper, we investigate Bianchi type- cosmological model for the universe filled with dark energy and viscous fluid in the presence of cosmological constant. Also, we show accelerating expansion of the universe by drawing volume scale, pressure and energy density versus cosmic time. In order to solve the Einstein field equations, we assume the expansion scalar is proportional to a component of the shear tensor. Therefore, we obtain the directional scale factors and show the EOS parameter crosses over phantom divided-line.
Keywords
Cite
@article{arxiv.1308.5308,
title = {Stability of viscous fluid in Bianchi type-VI model with cosmological constant},
author = {J. Sadeghi and Ali R. Amani and N. Tahmasbi},
journal= {arXiv preprint arXiv:1308.5308},
year = {2013}
}
Comments
12 pages, 7 Postscript figures