Octant sensitivity for large theta(13) in atmospheric and long baseline neutrino experiments
Animesh Chatterjee, Pomita Ghoshal, Srubabati Goswami, Sushant K. Raut

TL;DR
This paper evaluates the potential of long baseline and atmospheric neutrino experiments to determine the octant of theta_{23} in light of recent measurements of theta_{13}, highlighting the benefits of combined data for improved sensitivity.
Contribution
It analyzes how combining T2K, NOvA, and atmospheric neutrino data enhances octant sensitivity for theta_{23} considering recent theta_{13} measurements.
Findings
Combined experiments can achieve up to 4 sigma sensitivity for theta_{23} octant.
Atmospheric neutrino detectors significantly improve octant determination.
Sensitivity depends on hierarchy, delta_{CP}, and detector technology.
Abstract
One of the unknown parameters in neutrino oscillations is the octant of the mixing angle theta_{23}. In this paper, we discuss the possibility of determining the octant of theta_{23} in the long baseline experiments T2K and NOvA in conjunction with future atmospheric neutrino detectors, in light of non-zero value of theta_{13} measured by reactor experiments. We consider two detector technologies for atmospheric neutrinos - magnetized iron calorimeter and non-magnetized Liquid Argon Time Projection Chamber. We present the octant sensitivity for T2K/NOvA and atmospheric neutrino experiments separately as well as combined. For the long baseline experiments, a precise measurement of theta_{13}, which can exclude degenerate solutions in the wrong octant, increases the sensitivity drastically. For theta_{23} = 39^o and sin^2 2 theta_{13} = 0.1, at least ~2 sigma sensitivity can be achieved…
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