Pinning down neutrino oscillation parameters in the 2-3 sector with a mgnetised atmospheric neutrino detector: a new study

Abstract

We determine the sensitivity to neutrino oscillation parameters from a study of atmospheric neutrinos in a magnetised detector such as the ICAL at the proposed India-based Neutrino Observatory. In such a detector that can {\em separately} count ${\nu }_{\mu }$ and ${\overline{\nu }}_{\mu }$-induced events, the relatively smaller (about 5\%) uncertainties on the neutrino--anti-neutrino flux ratios translate to a constraint in the ${\chi }^2$ analysis that results in a significant improvement in the precision with which neutrino oscillation parameters such as ${\sin }^2{\theta }_{23}$ can be determined. Such an effect is unique to all magnetisable detectors and constitutes a great advantage in determining neutrino oscillation parameters using such detectors. Such a study has been performed for the first time here. Along with an increase in the kinematic range compared to earlier analyses, this results in sensitivities to oscillation parameters in the 2--3 sector that are comparable to or better than those from accelerator experiments where the fluxes are significantly higher. For example, the $1\sigma$ precisions on ${\sin }^2{\theta }_{23}$ and $|\Delta m_{32(31)}^2|$ achievable for 500 kTon yr exposure of ICAL are $\sim 9\%$ and $\sim 2.5\%$ respectively for both normal and inverted hierarchies. The mass hierarchy sensitivity achievable with this combination when the true hierarchy is normal (inverted) for the same exposure is $\Delta {\chi }^2\approx 8.5$ ($\Delta {\chi }^2\approx 9.5$).