Chaotic inflation with a fractional power-law potential in strongly coupled gauge theories

被引:41
|
作者
Harigaya, Keisuke [1 ]
Ibe, Masahiro [1 ,2 ]
Schmitz, Kai [1 ]
Yanagida, Tsutomu T. [1 ]
机构
[1] Univ Tokyo, Kavli IPMU, TODIAS, Kashiwa, Chiba 2778583, Japan
[2] Univ Tokyo, ICRR, Kashiwa, Chiba 2778582, Japan
关键词
DYNAMICAL SUPERSYMMETRY BREAKING; FLATNESS; UNIVERSE; HORIZON; MODELS; VACUA;
D O I
10.1016/j.physletb.2013.01.058
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Models of chaotic inflation with a fractional power-law potential are not only viable but also testable in the foreseeable future. We show that such models can be realized in simple strongly coupled supersymmetric gauge theories. In these models, the energy scale during inflation is dynamically generated by the dimensional transmutation due to the strong gauge dynamics. Therefore, such models not only explain the origin of the fractional power in the inflationary potential but also provide a reason why the energy scale of inflation is much smaller than the Planck scale. (C) 2013 Elsevier B.V. All rights reserved.
引用
收藏
页码:125 / 129
页数:5
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