Abstract
We study dependence of the atmospheric νμ and \( {\bar{\nu }_\mu } \) fluxes on the deviations of the 2–3 mixing from maximal, |45° − θ 23|, on the θ 23-octant and on the neutrino mass splitting ∆m 232 . Analytic expressions for the θ 23-deviation effect and the octant asymmetry are derived. We present conservative estimations of sensitivities of the iron (magnetized) calorimeter detectors (ICAL) to these parameters. ICAL can establish the θ 23-deviation at higher than 3σ confidence level if |45° − θ 23| > 6° with the exposure of 1 Mton·yr. Sensitivity to the octant is low for zero or very small 1–3 mixing, but it can be substantially enhanced for θ 13 > 3°. ICAL can measure the difference of ∆m 232 in ν and \( \bar{\nu } \) channels (the CPT test) with accuracy 0.8 × 10−4 eV2 (3σ) with 1 Mton·yr exposure, and the present MINOS result can be excluded at > 5σ confidence level. We discuss possible ways to further improve sensitivity of the magnetized spectrometers.
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Samanta, A., Smirnov, A.Y. The 2–3 mixing and mass split: atmospheric neutrinos and magnetized spectrometers. J. High Energ. Phys. 2011, 48 (2011). https://doi.org/10.1007/JHEP07(2011)048
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DOI: https://doi.org/10.1007/JHEP07(2011)048