Atmospheric neutrino challenges
arXiv:astro-ph/0412395 · doi:10.1016/j.nuclphysbps.2005.03.038
Abstract
We briefly review the improvements in the predictions of atmospheric neutrino fluxes since the NOW2000 workshop. In spite of the great progress in calculational technique the predictions are still not exact because of the uncertainties in the two major sets of input - cosmic ray flux and hadronic interactions on light nuclei.
6 pages, 7 postscript figures, prepared for the NOW 2004 Proceedings
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