Identifying the Neutrino mass Ordering with INO and NOvA

Details Identifying the Neutrino mass Ordering with INO and NOvA Identifying the Neutrino mass Ordering with INO and NOvA

2012-03-15

arxiv.org/abs/1203.3388v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

17 pages, 8 figures

Scientific paper

The relatively large value of $\theta_{13}$ 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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