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arXiv · 2409.10880

Estimation of the composition of ultra-high energy cosmic rays using the muon correlation method based on Yakutsk EAS array data

A. V. Glushkov·L. T. Ksenofontov·K. G. Lebedev·A. Sabourov
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Abstract

In this article a new method is proposed for estimating the mass composition of cosmic rays in individual events with energies above $1.25 \times 10^{19}$ eV. It is based on a joint analysis of experimental data and simulation results obtained using the QGSJet-II.04 model for muons with threshold energy $E_{\mu} = 1.0 \times \cos\theta$ GeV in air showers with zenith angles up to 60 degrees. The data from ground-based and underground scintillation detectors of the Yakutsk EAS array were used. Separate groups of nuclei and other primary particles were found.

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A. V. Glushkov, L. T. Ksenofontov, K. G. Lebedev, A. Sabourov. 2024-09-17. Estimation of the composition of ultra-high energy cosmic rays using the muon correlation method based on Yakutsk EAS array data. https://arxiv.org/abs/2409.10880

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