Cosmological models with the spinor and non-minimally interacting scalar field
General Relativity and Quantum Cosmology
2015-06-23 v1
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.
Keywords
Cite
@article{arxiv.1411.5445,
title = {Cosmological models with the spinor and non-minimally interacting scalar field},
author = {K. E. Osetrin and A. N. Makarenko and Yu. A. Rybalov},
journal= {arXiv preprint arXiv:1411.5445},
year = {2015}
}
Comments
9 pages, 2 figures, to appear Modern Physics Letters A