Mass composition of cosmic rays determined by the muon fraction with ϵthr1GeV in air showers with energy greater than 5 EeV

S. P. Knurenko and I. S. Petrov
Phys. Rev. D 102, 023036 – Published 28 July 2020

Abstract

The ratio of the number of muons with a threshold of 1 GeV and charged particles at a distance of 600 m from the axis is analyzed. Air showers with energies above 5 EeV and zenith angles with less than 60 degrees are considered. Comparison of experimental data with calculations by the QGSJETII-04 model for various primary nuclei, including a gamma ray, showed that the mass composition of cosmic rays up to energies of 10EeV mainly consists of protons and helium nuclei, with a small number of heavy nuclei. Data include air showers with a very low muon content, which are assumed to be produced by primary gamma rays.

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  • Received 29 April 2020
  • Accepted 9 July 2020

DOI:https://doi.org/10.1103/PhysRevD.102.023036

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear PhysicsGravitation, Cosmology & Astrophysics

Authors & Affiliations

S. P. Knurenko and I. S. Petrov*

  • Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy, 31 Lenin Avenue, 677980, Yakutsk, Russia

  • *Corresponding author. igor.petrov@ikfia.ysn.ru
  • knurenko@ikfia.ysn.ru

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Vol. 102, Iss. 2 — 15 July 2020

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