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- W2006300935 abstract "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." @default.
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- W2006300935 date "2015-02-03" @default.
- W2006300935 modified "2023-09-25" @default.
- W2006300935 title "Cosmological models with the spinor and non-minimally interacting scalar field" @default.
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- W2006300935 doi "https://doi.org/10.1142/s0217732315500157" @default.
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