Flux of upward high-energy muons at the multi-component primary energy spectrum
classification
✦ hep-ph
keywords
energyatmosphericfluxmulti-componentmuonprimaryrangespectrum
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The atmospheric neutrino-induced upward muon flux are calculated by using the multi-component primary energy spectrum, CORSIKA EAS simulation code for the reproduction of the atmospheric neutrino spectra and improved parton model for charged-current cross sections. The results are obtained at 0.1-1000 TeV muon energy range and 0-89 degrees zenith angular range.
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