Self-consistency of interaction models QGSJET 01, SIBYLL 2.1, NEXUS 3.97 and QGSJET II is checked in terms of their ability to reproduce simultaneously experimental data on fluxes of muons and hadrons. From this point of view SIBYLL 2.1 gives the most acceptable, though not quite satisfactory, results. Analysis of the situation for muons supports our previous conclusions, that high-energy muon deficit is due both to underestimation of primary light nuclei fluxes in direct emulsion chamber experiments and to softness of $p+A\to\pi^\pm,K^\pm+X$ inclusive spectra in fragmentation region, especially prominent in case of QGSJET 01 model
Over the last two decades, various experiments have measured muon densities in extensive air showers...
The evolution of the muon content of very high energy air showers (EAS) in the atmosphere is investi...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
Uncertainties of the model energy spectra of the most energetic secondary charged mesons are discuss...
We present a summary of recent tests and measurements of hadronic interaction properties with air sh...
Recent results obtained from leading cosmic ray experiments indicate that simulations using LHC-tune...
Monte Carlo simulations of extensive air showers were performed using a couple of different nuclear ...
More accurate original calculations of the atmospheric vertical muon energy spectra at energies 102 ...
More accurate original calculations of the atmospheric vertical muon energy spectra at energies 102 ...
The recent observations of muon charge ratio up to about 10 TeV and of atmospheric neutrinos up to e...
The Sydney University Giant Air-shower Recorder (SUGAR) measured the energy spectrum of ultra-high-e...
The quark-gluon strings model succeeds in the description of multiple hadron production in the centr...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
Abstract: The atmospheric muon fluxes at different zenith angles are calculated in the energy region...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
The evolution of the muon content of very high energy air showers (EAS) in the atmosphere is investi...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
Uncertainties of the model energy spectra of the most energetic secondary charged mesons are discuss...
We present a summary of recent tests and measurements of hadronic interaction properties with air sh...
Recent results obtained from leading cosmic ray experiments indicate that simulations using LHC-tune...
Monte Carlo simulations of extensive air showers were performed using a couple of different nuclear ...
More accurate original calculations of the atmospheric vertical muon energy spectra at energies 102 ...
More accurate original calculations of the atmospheric vertical muon energy spectra at energies 102 ...
The recent observations of muon charge ratio up to about 10 TeV and of atmospheric neutrinos up to e...
The Sydney University Giant Air-shower Recorder (SUGAR) measured the energy spectrum of ultra-high-e...
The quark-gluon strings model succeeds in the description of multiple hadron production in the centr...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
Abstract: The atmospheric muon fluxes at different zenith angles are calculated in the energy region...
Over the last two decades, various experiments have measured muon densities in extensive air showers...
The evolution of the muon content of very high energy air showers (EAS) in the atmosphere is investi...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...