arXiv · 1203.3388
Identifying the Neutrino mass Ordering with INO and NOvA
Abstract
The relatively large value of $θ_{13}$ established recently by the Daya Bay reactor experiment opens the possibility to determine the neutrino mass ordering with experiments currently under construction. We investigate synergies between the NOvA long-baseline accelerator experiment with atmospheric neutrino data from the India-based Neutrino Observatory (INO). We identify the requirements on energy and direction reconstruction and detector mass for INO necessary for a significant sensitivity. If neutrino energy and direction reconstruction at the level of 10% and 10 degree can be achieved by INO a determination of the neutrino mass ordering seems possible around 2020.
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Mattias Blennow, Thomas Schwetz. 2012-10-24. Identifying the Neutrino mass Ordering with INO and NOvA. https://doi.org/10.1007/jhep08(2012)058
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