Inflationary magnetogenesis with broken local U(1) symmetry

被引:15
|
作者
Domenech, Guillem [1 ]
Lin, Chunshan [1 ]
Sasaki, Misao [1 ]
机构
[1] Kyoto Univ, Yukawa Inst Theoret Phys, Ctr Gravitat Phys, Sakyo Ku, Kitashirakawa Oiwakecho, Kyoto 6068502, Japan
关键词
INTERGALACTIC MAGNETIC-FIELD; TEV BLAZARS; PERTURBATIONS; GENERATION; UNIVERSE;
D O I
10.1209/0295-5075/115/19001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We point out that a successful inflationary magnetogenesis could be realised if we break the local U(1) gauge symmetry during inflation. The effective electric charge is fixed as a fundamental constant, which allows us to obtain an almost scale-invariant magnetic spectrum avoiding both the strong coupling and back reaction problems. We examine the corrections to the primordial curvature perturbation due to these stochastic electromagnetic fields and find that, at both linear and non-linear orders, the contributions from the electromagnetic field are negligible compared to those created from vacuum fluctuations. Finally, the U(1) gauge symmetry is restored at the end of inflation. Copyright (C) EPLA, 2016
引用
收藏
页数:5
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