Abstract

Atmospheric muons of high energy constitute the major event yield in modern deep large-volume neutrino telescopes. Examining their properties at sea level is crucial for accurately deciphering observed signals. This study involves the computation of the flux and charge ratio of the atmospheric muons with energies exceeding 100 GeV at sea level. The calculation employs the Monte Carlo code CORSIKA in conjunction with several state-of-the-art hadronic interaction models. The obtained results are compared with a set of experimental data and with other recent comparable studies.

中文翻译：

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海平面高能大气 μ 子的通量和电荷比的计算*

摘要

大气高能μ子构成了现代深海大体积中微子望远镜的主要事件产量。在海平面检查它们的特性对于准确破译观测到的信号至关重要。这项研究涉及海平面能量超过100 GeV的大气μ介子的通量和电荷比的计算。该计算采用蒙特卡洛代码 CORSIKA 与几个最先进的强子相互作用模型相结合。将获得的结果与一组实验数据以及其他最近的可比研究进行比较。