Tilted Bianchi Type I Cosmological Models Filled with Disordered Radiation in General Relativity Revisited
arXiv:gr-qc/0212108 · doi:10.1023/A:1026301915781
Abstract
Tilted Bianchi type I cosmological models filled with disordered radiation 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 properties of the models are also discussed.
12 pages