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.
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Pradhan, A., Rai, A. Tilted Bianchi type I cosmological models filled with disordered radiation in general relativity revisitedD. Astrophysics and Space Science 286, 347–358 (2003). https://doi.org/10.1023/A:1026301915781
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DOI: https://doi.org/10.1023/A:1026301915781