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A Monte Carlo Calculation of Atmospheric Muon and Neutrino Fluxes

M. Thunman·G. Ingelman·P. Gondolo
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Abstract

Production of muons and neutrinos in cosmic ray interactions with the atmosphere has been investigated with a cascade simulation program based on Lund Monte Carlo programs. The resulting `conventional' muon and neutrino fluxes (from $π,K$ decays) agree well with earlier calculations, whereas the improved charm particle treatment used in this study gives significantly lower `prompt' fluxes compared to earlier estimates. This implies better prospects for detecting very high energy neutrinos from cosmic sources.

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M. Thunman, G. Ingelman, P. Gondolo. 1995-02-28. A Monte Carlo Calculation of Atmospheric Muon and Neutrino Fluxes. https://doi.org/10.1016/0920-5632(95)00489-v

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