Tilted Bianchi Type V Bulk Viscous Cosmological Models in General Relativity
arXiv:gr-qc/0307045 · doi:10.1023/B:astr.0000032069.58003.b4
Abstract
Conformally flat tilted Bianchi type V cosmological models in presence of a bulk viscous fluid and heat flow are investigated. The coefficient of bulk viscosity is assumed to be a power function of mass density. Some physical and geometric aspects of the models are also discussed.
14 pages