Inflation with massive vector fields

被引:15
作者
Liu, Junyu [1 ]
Wang, Yi [2 ]
Zhou, Siyi [2 ]
机构
[1] Univ Sci & Technol China, Hefei 230026, Anhui, Peoples R China
[2] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2015年 / 08期
基金
欧洲研究理事会;
关键词
inflation; physics of the early universe; cosmological perturbation theory; PERTURBATIONS; FLATNESS; UNIVERSE; HORIZON;
D O I
10.1088/1475-7516/2015/08/033
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the coupling between the inflaton and massive vector fields. All renormalizable couplings with shift symmetry of the inflaton are considered. The massive vector can be decomposed into a scalar mode and a divergence-free vector mode. We show that the former naturally interacts with the inflaton and the latter decouples at tree level. The model in general predicts f(NL)(equil) = O(1), while in some regions of the parameter space large non-Gaussianity can arise.
引用
收藏
页数:20
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