Higgs inflation and Higgs portal dark matter with right-handed neutrinos

被引:7
|
作者
Haba, Naoyuki [1 ]
Ishida, Hiroyuki [1 ]
Takahashi, Ryo [1 ]
机构
[1] Shimane Univ, Grad Sch Sci & Engn, Matsue, Shimane 6908504, Japan
来源
基金
日本学术振兴会;
关键词
STANDARD MODEL; BOSON;
D O I
10.1093/ptep/ptv053
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate the Higgs inflation and the Higgs portal dark matter with the right- handed neutrino. The dark matter and the right- handed neutrino in the Higgs inflation play important roles in explaining the recent experimental results of the Higgs and top masses, and the cosmic microwave background by BICEP2 at the same time. This inflation model predicts 805 GeV less than or similar to m(DM) less than or similar to 1220 GeV for the DM mass, 1.05 x 10(14) GeV less than or similar to MR less than or similar to 2.04 x 10(14) GeV for the right- handed neutrino mass, and 8.42 less than or similar to xi less than or similar to 12.4 for the non- minimal coupling within m(H) = 125.6 +/- 0.35 GeV for the Higgs and M-t = 173.34 +/- 0.76 GeV for the top masses.
引用
收藏
页数:10
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