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Local Muon Density Spectra at Various Zenith Angles Measured with NEVOD-DECOR

机译:用Nevod装饰测量的各种天顶角的局部μ子密度光谱

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摘要

Data on cosmic ray muon bundles accumulated at the NEVOD-DECOR complex over the period from May 2012 to December 2018 have been analyzed. Local muon density spectra at various zenith angles have been reconstructed and compared with CORSIKA-based simulations. At large zenith angles and high muon multiplicities corresponding to primary particle energies more than about 3 x 10(17) eV an excess of multi-muon events compared to simulations is clearly seen. Present data are compatible with the expectation for recent LHC-adjusted hadron interaction models only under assumption of extremely heavy (iron group nuclei) primary composition. The assumption of a heavy composition is however in contradiction with other EAS observables, such as maximum depth and its fluctuations.
机译:已经分析了2012年5月至2018年12月在Nevod-Decor Complex堆积的宇宙射线袋的数据已经分析到2018年5月至2018年12月。 已经重建了各种天性角度的局部μ子密度光谱,并与基于Corsika的模拟相比。 在大的天顶角度和高μ子倍数对应于大约3×10(17)的主要粒子能量,显然是与模拟相比的多μ子事件。 目前的数据与最近的LHC调整后的HOTRON相互作用模型的期望兼容,仅在极其重(铁组核)主要组合物的假设下。 然而,重型组合物的假设与其他EAS可观察到的可观察到,例如最大深度及其波动等矛盾。

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