Dark matter, shared asymmetries, and galactic gamma ray signals

被引:16
作者
Fonseca, Nayara [1 ,2 ]
Necib, Lina [2 ]
Thaler, Jesse [2 ]
机构
[1] Univ Sao Paulo, Inst Fis, BR-05508900 Sao Paulo, SP, Brazil
[2] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2016年 / 02期
基金
巴西圣保罗研究基金会;
关键词
dark matter theory; dark matter experiments; baryon asymmetry; gamma ray experiments; STABLE PARTICLES; NUMBER;
D O I
10.1088/1475-7516/2016/02/052
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We introduce a novel dark matter scenario where the visible sector and the dark sector share a common asymmetry. The two sectors are connected through an unstable mediator with baryon number one, allowing the standard model baryon asymmetry to be shared with dark matter via semi-annihilation. The present-day abundance of dark matter is then set by thermal freeze-out of this semi-annihilation process, yielding an asymmetric version of the WIMP miracle as well as promising signals for indirect detection experiments. As a proof of concept, we find a viable region of parameter space consistent with the observed Fermi excess of GeV gamma rays from the galactic center.
引用
收藏
页数:35
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