Cosmological models with the spinor and non-minimally interacting scalar   field
  The solution to the current extending Universe problem, and the description of all stages of evolution compels scientists to consider various cosmological models. Scalar - tensor models are rather simple and also allow us to clearly define the separate stages of evolution. Furthermore, other cosmological models are reduced. Our work takes into consideration the non-minimally interacted scalar field and the spinor field. The spinor field has been considered to establish a better understanding of the stages of evolution in our Universe. 
K.E. Osetrin, A.N. Makarenko and Yu.A. Rybalov
gr-qc