Inconsistencies in Interpreting the Atmospheric Neutrino Anomaly
arXiv:hep-ph/0305022 · doi:10.1007/BF02705334
Abstract
We note a discrepancy between the value of R expected on the basis of the muon neutrino angular distribution and the value actually observed. The energy independence of leads to a fine tuning problem. This may be indicative of some unaccounted for new physics.
3 pages, 5 figures