Enhancing the hierarchy and octant sensitivity of ESSSB in conjunction with T2K, NOA and ICAL@INO
arXiv:1902.02963 · doi:10.1007/JHEP05(2019)137
Abstract
The main aim of the ESSSB proposal is the discovery of the leptonic CP phase with a high significance ( for 50% values of ) by utilizing the physics at the second oscillation maxima of the channel. It can achieve sensitivity to hierarchy for all values of . In this work, we concentrate on the hierarchy and octant sensitivity of the ESSSB experiment. We show that combining the ESSSB experiment with the atmospheric neutrino data from the proposed India-based Neutrino Observatory(INO) experiment can result in an increased sensitivity to mass hierarchy. In addition, we also combine the results from the ongoing experiments T2K and NOA assuming their full runtime and present the combined sensitivity of ESSSB + ICAL@INO + T2K + NOA. We show that while by itself ESSSB can have up to hierarchy sensitivity, the combination of all the experiments can give up to sensitivity depending on the true hierarchy-octant combination. The octant sensitivity of ESSSB is low by itself. However the combined sensitivity of all the above experiments can give up to sensitivity depending on the choice of true hierarchy and octant. We discuss the various degeneracies and the synergies that lead to the enhanced sensitivity when combining different experimental data.
7 figures, 4 tables, minor typos corrected, updated to the published version
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