Prospects for Light Dark Matter Searches at Large-Volume Neutrino Detectors

被引:3
|
作者
Dutta, Bhaskar [1 ]
Huang, Wei-Chih [1 ]
Kim, Doojin [1 ,2 ]
Newstead, Jayden L. [3 ]
Park, Jong-Chul [4 ,5 ]
Ali, Iman Shaukat [3 ]
机构
[1] Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, Dept Phys & Astron, College Stn, TX 77843 USA
[2] Univ South Dakota, Dept Phys, Vermillion, SD 57069 USA
[3] Univ Melbourne, ARC Ctr Excellence Dark Matter Particle Phys, Sch Phys, Parkville, Vic 3010, Australia
[4] Chungnam Natl Univ, Dept Phys, Daejeon 34134, South Korea
[5] Chungnam Natl Univ, Inst Quantum Syst IQS, Daejeon 34134, South Korea
基金
澳大利亚研究理事会; 新加坡国家研究基金会;
关键词
HIGH-RESOLUTION E; E'; OXYGEN ISOTOPES; M2; TRANSITIONS; ISOVECTOR M1; BOREXINO;
D O I
10.1103/PhysRevLett.133.161801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a new approach to search for light dark matter (DM), with keV-GeV mass, via inelastic nucleus scattering at large-volume neutrino detectors such as Borexino, DUNE, Super-K, Hyper-K, and JUNO. The approach uses inelastic nuclear scattering of cosmic-ray boosted DM, enabling a lowbackground search for DM in these experiments. Large neutrino detectors, with higher thresholds than dark matter detectors, can be used, since the nuclear deexcitation lines are O(10) MeV. Using a hadrophilic dark-gauge-boson-portal model as a benchmark, we show that the nuclear inelastic channels generally provide better sensitivity than the elastic scattering for a large region of light DM parameter space.
引用
收藏
页数:8
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