Embedding cosmological inflation, axion dark matter and seesaw mechanism in a 3-3-1 gauge model

被引：11
|
作者：
Ferreira, J. G., Jr. [1 ]
Pires, C. A. de S. [1 ]
Rodrigues, J. G. [1 ]
Rodrigues da Silva, P. S. [1 ]
机构：
[1] Univ Fed Paraiba, Dept Fis, Caixa Postal 5008, BR-58051970 Joao Pessoa, Paraiba, Brazil
来源：
PHYSICS LETTERS B | 2017年 / 771卷
关键词：
RADIATIVE-CORRECTIONS; INVARIANCE; MASSES;
D O I：
10.1016/j.physletb.2017.05.034
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Peccei-Quinn symmetry is an intrinsic global symmetry of the 3-3-1 gauge models. Its spontaneous breaking mechanism engendering an invisible KSVZ-like axion links the 3-3-1 models with new physics at similar to 10(10) GeV scale. The axion that results from this mechanism is an interesting candidate for the dark matter of the universe, while its real partner may drive inflation if radiative corrections are taken into account. This is obtained by connecting the type I seesaw mechanism with the spontaneous breaking of the Peccei-Quinn symmetry. In the end of the day we have a scenario providing a common answer to the strong-CP problem, inflation, dark matter and neutrino mass. (C) 2017 The Author(s). Published by Elsevier B.V.
引用
收藏
页码：199 / 205
页数：7
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