Energy spectrum and mass composition of the primary cosmic rays based on the intensity of muon bundles detected in the NEVOD-DECOR experiment

The article presents the results of analysis conducted on the NEVOD-DECOR data that were obtained following the study of inclined muon bundles ($\ensuremath{\theta}=40--85\ifmmode^\circ\else\textdegree\fi{}$) of cosmic rays for the time period from 2012 to 2023. The research was executed using original method for studying the extensive air showers, local muon density spectra. The data were compared with the calculations based on the simulation of air showers using the CORSIKA program for different models of hadronic interactions. The obtained estimates of the energy spectrum and the behavior of the mass composition of primary cosmic rays in a wide energy range from $2\ifmmode\times\else\texttimes\fi{}{10}^{15}$ to $3\ifmmode\times\else\texttimes\fi{}{10}^{18}\text{ }\text{ }\mathrm{eV}$ were compared with the data from other experiments.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-11-20
DOI
https://doi.org/10.1103/clp6-bp28
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

Energy spectrum and mass composition of the primary cosmic rays based on the intensity of muon bundles detected in the NEVOD-DECOR experiment

К. Г. Компаниец, А. А. Петрухин, G. Trinchero, G. Mannocchi et al.
Physical review. D/Physical review. D.
Astrophysics and Cosmic Phenomena
article

Energy spectrum and mass composition of the primary cosmic rays based on the intensity of muon bundles detected in the NEVOD-DECOR experiment

К. Г. Компаниец, А. А. Петрухин, G. Trinchero, G. Mannocchi, I. I. Yashin, I. A. Shulzhenko, E. A. Yurina, V. V. Kindin, A. Bogdanov, В. В. Шутенко, I. Yu. Troshin, С. С. Хохлов, V. S. Vorobyev, D. M. Gromushkin, A. Chiavassa, K. I. Mannanova, A. Yu. Konovalova
article en

Abstract

The article presents the results of analysis conducted on the NEVOD-DECOR data that were obtained following the study of inclined muon bundles ($\ensuremath{\theta}=40--85\ifmmode^\circ\else\textdegree\fi{}$) of cosmic rays for the time period from 2012 to 2023. The research was executed using original method for studying the extensive air showers, local muon density spectra. The data were compared with the calculations based on the simulation of air showers using the CORSIKA program for different models of hadronic interactions. The obtained estimates of the energy spectrum and the behavior of the mass composition of primary cosmic rays in a wide energy range from $2\ifmmode\times\else\texttimes\fi{}{10}^{15}$ to $3\ifmmode\times\else\texttimes\fi{}{10}^{18}\text{ }\text{ }\mathrm{eV}$ were compared with the data from other experiments.

Physical review. D/Physical review. D.Vol. 112(10)
Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Osservatorio Astrofisico di Torino (IT), University of Turin (IT), National Research Nuclear University MEPhI (RU)
Openalex Percentile: Top 84%
Astrophysics and Cosmic Phenomena
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