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 cosmolo...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2014-11
Main Authors: Osetrin, K E, Makarenko, A N, Rybalov, Yu A
Format: Article
Language:English
Subjects:
Astronomical models
Cosmology
Evolution
Magma
Star & galaxy formation
Tensors
Universe
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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.
ISSN:2331-8422
DOI:10.48550/arxiv.1411.5445