Dark matter origins of neutrino masses

被引:14
|
作者
Huang, Wei-Chih [1 ]
Deppisch, Frank F. [1 ]
机构
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
来源
PHYSICAL REVIEW D | 2015年 / 91卷 / 09期
基金
欧洲研究理事会;
关键词
D O I
10.1103/PhysRevD.91.093011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a simple scenario that directly connects the dark matter (DM) and neutrino mass scales. Based on an interaction between the DM particle chi and the neutrino nu of the form chi chi nu nu/Lambda(2), the DM annihilation cross section into the neutrino is determined and a neutrino mass is radiatively induced. Using the observed neutrino mass scale and the DM relic density, the DM mass and the effective scale. are found to be of the order MeV and GeV, respectively. We construct an ultraviolet-complete toy model based on the inverse seesaw mechanism which realizes this potential connection between DM and neutrino physics.
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页数:5
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