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

Fuente: arXiv
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Autores principales: Glushkov, A. V., Ksenofontov, L. T., Lebedev, K. G., Sabourov, A.
Formato: Preprint
Publicado: 2024
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author Glushkov, A. V.
Ksenofontov, L. T.
Lebedev, K. G.
Sabourov, A.
author_facet Glushkov, A. V.
Ksenofontov, L. T.
Lebedev, K. G.
Sabourov, A.
contents 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 $E_μ = 1.0 \times \cosθ$ 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.
format Preprint
id arxiv_https___arxiv_org_abs_2409_10880
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Estimation of the composition of ultra-high energy cosmic rays using the muon correlation method based on Yakutsk EAS array data
Glushkov, A. V.
Ksenofontov, L. T.
Lebedev, K. G.
Sabourov, A.
High Energy Astrophysical Phenomena
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 $E_μ = 1.0 \times \cosθ$ 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.
title Estimation of the composition of ultra-high energy cosmic rays using the muon correlation method based on Yakutsk EAS array data
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2409.10880