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.
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页数：9
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