Abstract
The study of a self-consistent system of interacting spinor and scalar fields within the scope of a Bianchi type I (BI) gravitational field in the presence of a viscous fluid and Λ term has been carried out. The system of equations defining the evolution of the volume scale of BI universe, energy density, and corresponding Hubble constant has been derived. The system in question has been thoroughly studied qualitatively. Corresponding solutions are graphically illustrated. The system in question is also studied from the view point of blow up. It has been shown that the blow up takes place only in the presence of viscosity.
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