The cross sections for neutrino interactions with nucleons have been measured directly in accelerator experiments and through the zenith-angle and energy dependence of neutrino events at the IceCube Neutrino Observatory. Fluxes of high-energy neutrinos are produced at the Large Hadron Collider and by cosmic rays in the atmosphere. High-energy neutrinos also come from astrophysical and cosmic sources. The theory of neutrino interactions is reviewed. Current cross-section measurements and prospects for the future are discussed. The focus here is on neutrino interactions for energies larger than 1 TeV.

中文翻译：

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高能到超高能中微子相互作用

中微子与核子相互作用的横截面已在加速器实验中直接测量，并通过冰立方中微子天文台的中微子事件的天顶角和能量依赖性进行测量。高能中微子通量是由大型强子对撞机和大气中的宇宙射线产生的。高能中微子也来自天体物理和宇宙来源。回顾了中微子相互作用的理论。讨论了当前的横截面测量和未来的前景。这里的重点是能量大于 1 TeV 的中微子相互作用。