Author:
Datta Jaydeep,Singh Bana,Uma Sankar S.
Abstract
Abstract
We study the capability of INO-ICAL to determine the
neutrino oscillation parameters |ΔM
2
31| and
sin2
θ
23. We do not use any generator level
information. Instead, we process the generated atmospheric neutrino
events through GEANT4 simulation of the detector and the event
reconstruction framework. Among the outputs of this framework, only
the momentum and direction of the longest track were used in a
previous study by other authors. In this study, in addition to
these two variables, we consider a third variable based on
additional hits, which arise due to hadrons in the event. We show
that the inclusion of this variable leads to a 30% reduction in
the uncertainty of |ΔM
2
31| for a 5-year run of ICAL. We
find that doubling the exposure time leads to an additional 30%
reduction in the uncertainties of both |ΔM
2
31| and
sin2
θ
23.
Subject
Mathematical Physics,Instrumentation
Cited by
1 articles.
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