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arXiv · hep-ph/9812462

Atmospheric neutrinos from charm

L. Pasquali·M. H. Reno·I. Sarcevic
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Abstract

Using next-to-leading order perturbative QCD, we find that the charm contribution to the atmospheric lepton fluxes dominates over the conventional ones from pi and K decays for energies higher than 10^5 GeV. We also discuss theoretical uncertainties involved in the calculations and compare our results with previous evaluations.

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L. Pasquali, M. H. Reno, I. Sarcevic. 1998-12-21. Atmospheric neutrinos from charm. https://doi.org/10.1063/1.59421

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