Inconsistencies in Interpreting the Atmospheric Neutrino Anomaly

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dc.creatorLoSecco, John M.
dc.date2003-05-02
dc.date.accessioned2026-07-07T11:09:23Z
dc.date.available2026-07-07T11:09:23Z
dc.descriptionWe 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 $R$ leads to a fine tuning problem. This may be indicative of some unaccounted for new physics.
dc.description3 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0305022
dc.identifierhttp://arxiv.org/abs/hep-ph/0305022
dc.identifierPramana62:635-638,2004
dc.identifierdoi:10.1007/BF02705334
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190452
dc.subjectHigh Energy Physics - Phenomenology
dc.titleInconsistencies in Interpreting the Atmospheric Neutrino Anomaly
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