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 IceCube 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。高能中微子的通量是在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学和宇宙源。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。这里的重点是大于 1 TeV 的能量的中微子相互作用。