Abstract

There was a lot of puzzles in the history of the discovery and investigations of the muon itself and the muon component of cosmic rays. The last of them is an excess of high-multiplicity muon groups that grows with increasing energy of primary cosmic rays and which is detected in various experiments. An excess of muons that have ultrahigh energies (above 100 TeV) is the second aspect of the muon puzzle. Various approaches to solving the muon puzzle that are associated with measuring the energy features of the muon component of cosmic rays are considered.

中文翻译：

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宇宙射线中的μ子难题及其可能的解决方案

摘要

在对μ子本身和宇宙射线的μ子组成部分进行发现和研究的历史上，存在着许多困惑。它们中的最后一个是过量的高多重性介子基团，该基团随着初级宇宙射线能量的增加而增长，并且在各种实验中都可以检测到。拥有超高能量（超过100 TeV）的μ子是μ子难题的第二个方面。考虑了解决与测量宇宙射线的μ子分量的能量特征相关的μ子难题的各种方法。