IceCube events from heavy DM decays through the right-handed neutrino portal

被引:44
|
作者
Ko, P. [1 ]
Tang, Yong [1 ]
机构
[1] Korea Inst Adv Study, Sch Phys, Seoul 130722, South Korea
基金
新加坡国家研究基金会; 美国国家科学基金会;
关键词
HIGH-ENERGY NEUTRINOS; PARTICLE; ORIGIN;
D O I
10.1016/j.physletb.2015.10.021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The recently observed IceCube PeV events could be due to heavy dark matter (DM) decay. In this paper, we propose a simple DM model with extra U(1)(X) gauge symmetry and bridge it with standard model particles through heavy right-handed neutrino. The Dirac fermion DM chi with mass similar to 5PeV can dominantly decay into a dark Higgs (phi), the SM Higgs (h) and a neutrino (nu). If the lifetime of chi is similar to O(10(28)) s, the resulting neutrino flux can fit data consistently. The neutrino flux from chi ->phi h nu in our model is softer than the one predicted from chi ->nu h, for example. We also discuss a possible mechanism to produce DM with the right relic abundance. (C) 2015 The Authors. Published by Elsevier B.V.
引用
收藏
页码:81 / 88
页数:8
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