Light dark matter: Models and constraints

被引：266
作者：
Knapen, Simon [1 ,2 ]
Lin, Tongyan [1 ,2 ,3 ]
Zurek, Kathryn M. [1 ,2 ]
机构：
[1] Lawrence Berkeley Natl Lab, Theory Grp, Berkeley, CA 94709 USA
[2] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94709 USA
[3] Univ Calif San Diego, Dept Phys, San Diego, CA 92093 USA
来源：
PHYSICAL REVIEW D | 2017年 / 96卷 / 11期
关键词：
SEARCH; PARTICLES; AXIONS; DECAYS; BOSON;
D O I：
10.1103/PhysRevD.96.115021
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the direct detection prospects for a representative set of simplified models of sub-GeV dark matter (DM), accounting for existing terrestrial, astrophysical and cosmological constraints. We focus on dark matter lighter than an MeV, where these constraints are most stringent, and find three scenarios with accessible direct detection cross sections: (i) DM interacting via an ultralight kinetically mixed dark photon, (ii) a DM subcomponent interacting with nucleons or electrons through a light scalar or vector mediator, and (iii) DM coupled with nucleons via a mediator heavier than similar to 100 keV.
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页数：26
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