Dark matter through the axion portal

被引:181
|
作者
Nomura, Yasunori [1 ]
Thaler, Jesse
机构
[1] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA
来源
PHYSICAL REVIEW D | 2009年 / 79卷 / 07期
关键词
SEARCH;
D O I
10.1103/PhysRevD.79.075008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Motivated by the galactic positron excess seen by PAMELA and ATIC/PPB-BETS, we propose that dark matter is a TeV-scale particle that annihilates into a pseudoscalar "axion." The positron excess and the absence of an antiproton or gamma ray excess constrain the axion mass and branching ratios. In the simplest realization, the axion is associated with a Peccei-Quinn symmetry, in which case it has a mass around 360-800 MeV and decays into muons. We present a simple and predictive supersymmetric model implementing this scenario, where both the Higgsino and dark matter obtain masses from the same source of TeV-scale spontaneous symmetry breaking.
引用
收藏
页数:6
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