We study the sensitivity of the NO ν A near detector to MeV-GeV dark matter while operating symbiotically with the neutrino program. We find that NO ν A could explore a large new region of parameter space over the next few years for dark matter masses below 100?MeV, reaching the thermal target for a scalar dark matter particle for some masses. This result represents a significant improvement over existing probes such as BABAR , E137, MiniBooNE, and LSND.
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机译:我们与中微子程序共生时,研究了NO V A近探测器对MeV-GeV暗物质的敏感性。我们发现,对于低于100?MeV的暗物质质量,NO v A可以在未来几年内探索一个较大的参数空间新区域,从而达到某些质量的标量暗物质粒子的热目标。该结果表示相对于诸如BABAR,E137,MiniBooNE和LSND的现有探针有显着改进。
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