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Flux of upward high-energy muons at the multi-component primary energy spectrum

S. V. Ter-Antonyan·P. L. Biermann
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Abstract

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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S. V. Ter-Antonyan, P. L. Biermann. 2001-06-07. Flux of upward high-energy muons at the multi-component primary energy spectrum. https://arxiv.org/abs/hep-ph/0106076

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