Fluxes of vμ and ve in the atmosphere: Is there an anomaly?

Physics – Nuclear Physics

Scientific paper

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Scientific paper

There is a persistent discrepancy between the calculated and observed flavor ratio of cosmic ray neutrinos in the atmosphere, particularly in the energy region below 1 GeV. In this talk I review the status of calculations of atmospheric neutrinos and discuss possible interpretations in terms of neutrino oscillations. Limits from neutrino-induced upward muons are also considered.
Work supported in part by the U.S. Department of Energy under Grant DE-FG02-91ER40626.

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