High-energy cosmic ray fluxes in the Earth atmosphere: calculations vs experiments

Abstract

A new calculation of the atmospheric fluxes of cosmic-ray hadrons and muons in the energy range 10-10^5 GeV has been performed for the set of hadron production models, EPOS 1.6, QGSJET II-03, SIBYLL 2.1, and others that are of interest to cosmic ray physicists. The fluxes of secondary cosmic rays at several levels in the atmosphere are computed using directly data of the ATIC-2, GAMMA experiments, and the model proposed recently by Zatsepin and Sokolskaya as well as the parameterization of the primary cosmic ray spectrum by Gaisser and Honda. The calculated energy spectra of the hadrons and muon flux as a function of zenith angle are compared with measurements as well as other calculations. The effect of uncertainties both in the primary cosmic ray flux and hadronic model predictions on the spectra of atmospheric hadrons and muons is considered.

30 pages elsart, 18 figures; discussion extended, tables and references added, figures improved, typos corrected; final version accepted for publication in Astroparticle Physics

References in corpus (8)

• One-dimensional Hybrid Approach to Extensive Air Shower Simulation
• Spectrum of cosmic rays, produced in supernova remnants
• Rigidity-dependent cosmic ray energy spectra in the knee region obtained with the GAMMA experiment
• Hadronic Interactions at Cosmic Ray Energies
• Extended Air Shower Simulations Based on EPOS
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• Simulation of neutrino and charged particle production and propagation in the atmosphere
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Cited by in corpus (13)

• The Muon Puzzle in cosmic-ray induced air showers and its connection to the Large Hadron Collider
• The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes
• Influence of hadronic interaction models and the cosmic ray spectrum on the high energy atmospheric muon and neutrino flux
• Characterization of the Atmospheric Muon Flux in IceCube
• High-energy neutrino fluxes and flavor ratio in the Earth's atmosphere
• Atmospheric muon flux at PeV energies
• On the Accuracy of Underground Muon Intensity Calculations
• Data-driven hadronic interaction model for atmospheric lepton flux calculations
• High-energy atmospheric muon flux calculations in comparison with recent measurements
• Muons in IceCube
• Atmospheric Neutrinos
• Atmospheric Lepton Fluxes via Two-Dimensional Matrix Cascade Equations
• High-energy spectra of the atmospheric neutrinos: predictions and measurements