Muon puzzle in inclined muon bundles detected by NEVOD-DECOR

Aleksei Bogdanov, N. S. Barbashina, S. S. Khokhlov, V. V. Kindin, R. P. Kokoulin, K. G. Kompaniets, A. Y. Konovalova, G. Mannocchi, A. A. Petrukhin, V. V. Shutenko, G. Trinchero, V. S. Vorobev, I. I. Yashin, E. A. Yurina, E. A. Zadeba
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Abstract

The data of cosmic ray NEVOD-DECOR experiment on the investigation of inclined muon bundles for a long time period (May 2012 - March 2021) are presented. The analysis showed that the observed intensity of muon bundles at primary cosmic ray energies of about 1 EeV and higher can be compatible with the expectation in frame of widely used hadron interaction models only under the assumption of an extremely heavy mass composition. This conclusion is consistent with data of several experiments on investigations of muon content in air showers, but contradicts the available fluorescence data on X_{max} Xmax which favor a light mass composition at these energies. In order to clarify the nature of the "muon puzzle", investigations of the muon bundle energy deposit in the detector material were carried out. For the first time, experimental estimates of the average energy of muons in the bundles of inclined air showers initiated by primary particles with energies from 10 to 1000 PeV have been obtained.
NEVOD-DECOR探测到的倾斜μ子束中的μ子谜题
本文介绍了宇宙射线NEVOD-DECOR实验长期(2012年5月- 2021年3月)斜介子束研究的数据。分析表明,在一次宇宙射线能量约为1 EeV及以上的情况下,观测到的介子束强度只有在极重质量组成的假设下才能与广泛使用的强子相互作用模型框架下的期望相一致。这一结论与几个研究空气簇射中介子含量的实验数据是一致的,但与X_{max} Xmax的现有荧光数据相矛盾,后者倾向于这些能量下的轻质量组成。为了弄清“介子之谜”的本质,对探测器材料中的介子束能沉积进行了研究。本文首次获得了由10 ~ 1000 PeV的初级粒子引发的倾斜空气簇中介子平均能量的实验估计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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