Tilted Bianchi Type I Cosmological Models Filled with Disordered   Radiation in General Relativity Revisited
  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. 
Anirudh Pradhan and Abha Rai