Semi-analytic approximations for production of atmospheric muons and neutrinos

Astronomy and Astrophysics – Astrophysics

Scientific paper

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15 pages with 8 figures

Scientific paper

10.1016/S0927-6505(01)00143-8

Simple approximations for fluxes of atmospheric muons and muon neutrinos are
developed which display explicitly how the fluxes depend on primary cosmic ray
energy and on features of pion production. For energies of approximately 10 GeV
and above the results are sufficiently accurate to calculate response functions
and to use for estimates of systematic uncertainties.

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