ICANOE - Imaging and Calorimetric Neutrino Oscillation Experiment
A. Rubbia, ICARUS Collaboration, NOE Collaboration
TL;DR
ICANOE aims to clarify neutrino mass and mixing patterns by detecting CERN beam and cosmic ray events, providing independent measurements to refine oscillation parameters following SuperKamiokande findings.
Contribution
This paper introduces the ICANOE detector's approach for comprehensive neutrino oscillation studies using combined beam and cosmic ray data.
Findings
Independent measurements of oscillation parameters from CNGS and cosmic rays
Enhanced precision in neutrino mass and mixing pattern determination
Confirmation of SuperKamiokande results
Abstract
The main scientific goal of the ICANOE detector is the one of elucidating in a comprehensive way the pattern of neutrino masses and mixings, following the SuperKamiokande results and the observed solar neutrinos deficit. To achieve these goals, the experimental method is based upon the complementary and simultaneous detection of CERN beam (CNGS) and cosmic ray (CR) events. For the currently allowed values of the SuperKamiokande results, both CNGS and cosmic ray data will give independent measurements and provide a precise determination of the oscillation parameters.
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