Cosmological models with the spinor and non-minimally interacting scalar field

被引：0

作者：

Osetrin, K. E. ^{[1
]}

Makarenko, A. N. ^{[1
]}

Rybalov, Yu. A. ^{[1
,2
]}

机构：

[1] Tomsk State Pedag Univ, Tomsk, Russia

[2] Natl Res Tomsk State Univ, Tomsk, Russia

来源：

MODERN PHYSICS LETTERS A | 2015年 / 30卷 / 05期

关键词：

Cosmological model; non-minimally interactions; scalar field; PROBE WMAP OBSERVATIONS; ANGULAR POWER SPECTRUM; MODIFIED GRAVITY; DARK ENERGY; BOOMERANG; SUPERNOVAE; UNIVERSE; OMEGA;

D O I：

10.1142/S0217732315500157

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：9

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