Tilted Bianchi Type V Bulk Viscous Cosmological Models in General Relativity

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.

arXiv comment14 pages

References in corpus (3)

• Bulk Viscous Cosmology
• Bulk Viscous Solutions to the Field Equations and the Deceleration Parameter-Revisited
• Tilted Bianchi Type I Cosmological Models Filled with Disordered Radiation in General Relativity Revisited

Cited by in corpus (4)

• Cosmological constant dominated transit universe from early deceleration to current acceleration phase in Bianchi-V space-time
• Generation of Bianchi type V cosmological models with varying $\Lambda$-term
• Transit universe with time varying $G$ and decaying $\Lambda$
• The Momentum 4-Vector in Bulk Viscous Bianchi Type-V Space-time