Direct dark matter detection experiments will soon be sensitive to neutrinos from astrophysical sources, including the Sun, the atmosphere, and supernova. This sets an important benchmark for these experiments, and opens up a new window in neutrino physics and astrophysics. The detection of these neutrinos will be complementary to accelerator and reactor-based experiments which study neutrinos over the same energy range. Here we review the physics and astrophysics that can be extracted from the detection of these neutrinos, highlighting the potential for identifying new physics in the form of light mediators that arise from kinetic mixing and hidden sectors, and $\sim$ eV-scale sterile neutrinos. We discuss how the physics reach of these experiments will complement searches for new physics at the LHC and dedicated neutrino experiments.

中文翻译：

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暗物质探测器的中微子物理学

直接暗物质探测实验很快就会对来自天体物理来源（包括太阳、大气和超新星）的中微子敏感。这为这些实验设定了一个重要的基准，并为中微子物理学和天体物理学打开了一扇新窗口。这些中微子的探测将补充基于加速器和反应堆的实验，这些实验在相同的能量范围内研究中微子。在这里，我们回顾了可以从这些中微子的探测中提取的物理学和天体物理学，突出了以由动力学混合和隐藏扇区产生的光介质形式以及 $\sim$ eV 级无菌中微子的形式识别新物理学的潜力. 我们讨论了这些实验的物理范围将如何补充在 LHC 和专用中微子实验中寻找新物理。