Leptophilic dark matter confronts AMS-02 cosmic-ray positron flux

被引:10
|
作者
Cao, Qing-Hong [1 ,2 ,3 ,4 ]
Chen, Chuan-Ren [5 ]
Gong, Ti [1 ,2 ]
机构
[1] Peking Univ, Dept Phys, Beijing 100871, Peoples R China
[2] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
[3] Collaborat Innovat Ctr Quantum Matter, Beijing, Peoples R China
[4] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
[5] Natl Taiwan Normal Univ, Dept Phys, Taipei 116, Taiwan
基金
美国国家科学基金会;
关键词
SOLAR MODULATION; CONSTRAINTS; SPECTRUM; MODELS;
D O I
10.1016/j.cjph.2016.11.006
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
With the measurement of positron flux published recently by AMS-02 collaboration, we show how the leptophilic dark matter fits the observation. We obtain the percentages of different products of dark matter annihilation that can best describe the flux of high energy positrons observed by AMS. We show that dark matter annihilates predominantly into tau tau pair, while both ee and mu mu final states should be less than 20%. When gauge boson final states are included, the best branching ratio of needed tau tau mode reduces. (C) 2016 The Physical Society of the Republic of China (Taiwan). Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:10 / 15
页数:6
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