The sensitivity of the present CNGS beam to the sub-dominant ν μ â νe oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to θ13 of ICARUS and OPERA combined. We show that the CNGS beam optimized for Î½Ï appearance will improve significantly (about a factor of 5) the current limit of CHOOZ and explore most of the region sin2 2θ13 â O(10-2).
Komatsu, M., Migliozzi, P., Terranova, F. (2003). Sensitivity to θ13 of the CERN to Gran Sasso neutrino beam. JOURNAL OF PHYSICS. G, NUCLEAR AND PARTICLE PHYSICS, 29(2), 443-452 [10.1088/0954-3899/29/2/318].
Sensitivity to θ13 of the CERN to Gran Sasso neutrino beam
Terranova, F
2003
Abstract
The sensitivity of the present CNGS beam to the sub-dominant ν μ â νe oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to θ13 of ICARUS and OPERA combined. We show that the CNGS beam optimized for Î½Ï appearance will improve significantly (about a factor of 5) the current limit of CHOOZ and explore most of the region sin2 2θ13 â O(10-2).
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