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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.

preprint2014arXivOpen access
K. E. OsetrinA. N. MakarenkoYu. A. Rybalov
gr-qc
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Open access3 authors1 topic
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K. E. OsetrinA. N. MakarenkoYu. A. Rybalov

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