Sensitivity to neutrino mixing parameters with atmospheric neutrinos
Abhijit Samanta

TL;DR
This study analyzes atmospheric neutrino data using the ICAL detector to measure neutrino oscillation parameters, achieving significant precision in $ heta_{13}$, $ heta_{23}$, and $ ext{Δ}m_{32}^2$, and exploring octant discrimination.
Contribution
The paper introduces a detailed analysis method for atmospheric neutrinos with the ICAL detector, including new binning techniques and resolution functions, to improve measurement precision of oscillation parameters.
Findings
$ heta_{13}$ can be measured with significant precision.
$ ext{Δ}m_{32}^2$ and $ heta_{23}$ are measured with 8% and 38% accuracy.
Octant discrimination and deviation from maximal mixing are feasible.
Abstract
We have analyzed the atmospheric neutrino data to study the octant of and the precision of the oscillation parameters for a large Iron CALorimeter (ICAL) detector. The ICAL being a tracking detector has the ability to measure the energy and the direction of the muon with high resolution. From bending of the track in magnetic field it can also distinguish its charge. We have generated events by Nuance and then considered only the muons (directly measurable quantities) produced in charge current interactions in our analysis. This encounters the main problem of wide resolutions of energy and baseline. The energy-angle correlated two dimensional resolution functions are used to migrate the energy and the zenith angle of the neutrino to those of the muon. A new type of binning has been introduced to get better reflection of the oscillation pattern in chi-square analysis. Then…
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