Inconsistencies in interpreting the atmospheric neutrino anomaly
We note a discrepancy between the value ofR expected on the basis of the muon neutrino angular distribution and the value actually observed. The energy independence ofR leads to a fine-tuning problem. This may be indicative of some unaccounted for new physics.
KeywordsNeutrino atmospheric anomaly
PACS Nos14.60.Pq 14.60.St
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