Atmospheric neutrinos from charm

Details Atmospheric neutrinos from charm Atmospheric neutrinos from charm

1998-12-21

arxiv.org/abs/hep-ph/9812462v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

5 pages, 1 figure, submitted to the Proceedings of the International Workshop on Particle Physics and the Early Universe (COSM

Scientific paper

10.1063/1.59421

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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