中微子实验探测亲水的轻暗物质

Yohei Ema, F. Sala, R. Sato
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引用次数: 20

摘要

我们使用Super-K数据对亚gev暗物质(DM)与原子核的相互作用施加了新的强限制,这种相互作用依赖于宇宙射线向上散射不可避免地引起的DM通量。我们在Hyper-K和DUNE上得到了类似的灵敏度,并将它们与其他灵敏度进行了比较,例如朱诺。使用简化模型,我们发现我们的建议测试了真正的新参数空间,这是由理论一致性和其他直接探测实验、宇宙学、介子衰变和我们对单喷流的重铸所允许的。因此,我们的研究结果为任何对核反冲敏感的大体积探测器激发和塑造了一个新的物理案例。
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Neutrino experiments probe hadrophilic light dark matter
We use Super-K data to place new strong limits on interactions of sub-GeV Dark Matter (DM) with nuclei, that rely on the DM flux inevitably induced by cosmic-ray upscatterings. We derive analogous sensitivities at Hyper-K and DUNE and compare them with others, e.g. at JUNO. Using simplified models, we find that our proposal tests genuinely new parameter space, allowed both by theoretical consistency and by other direct detection experiments, cosmology, meson decays and our recast of monojet. Our results thus motivate and shape a new physics case for any large volume detector sensitive to nuclear recoils.
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