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Identifying the Neutrino mass Ordering with INO and NOvA

MPS-Authors
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Blennow,  Mattias
Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society;

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Schwetz-Mangold,  Thomas
Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society;

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フルテキスト (公開)

1203.3388
(プレプリント), 193KB

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引用

Blennow, M., & Schwetz-Mangold, T. (2012). Identifying the Neutrino mass Ordering with INO and NOvA. Journal of High Energy Physics, 2012(8):, pp. 1-16. doi:10.1007/JHEP08(2012)058.


引用: https://hdl.handle.net/11858/00-001M-0000-000F-F08D-6
要旨
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.