Neutrino Masses and Oscillations 2015
Vincenzo Flaminio 1 and Mauro Mezzetto 2 and Leslie Camilleri 3 and Srubabati Goswami 4 and Seon-Hee Seo 5 1, Physics Department and INFN, Pisa University, Largo B. Pontecorvo, 56127 Pisa, Italy 2, Physics Department and INFN, Padova University, Via Marzolo, 35131 Padova, Italy 3, Nevis Labs, Columb...
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Veröffentlicht in: | Advances in High Energy Physics 2017-01, Vol.2017, p.1-3 |
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Sprache: | eng |
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Zusammenfassung: | Vincenzo Flaminio 1 and Mauro Mezzetto 2 and Leslie Camilleri 3 and Srubabati Goswami 4 and Seon-Hee Seo 5 1, Physics Department and INFN, Pisa University, Largo B. Pontecorvo, 56127 Pisa, Italy 2, Physics Department and INFN, Padova University, Via Marzolo, 35131 Padova, Italy 3, Nevis Labs, Columbia University, P.O. Box 137, Irvington, NY 10533, USA 4, Physical Research Laboratory, Navrangpura, Ahmedabad 380009, India 5, Department of Physics and Astronomy, Seoul National University, 1 Gwenak-ro, Gwenak-gu, Seoul 08826, Republic of Korea Received 25 February 2016; Accepted 25 February 2016; 13 February 2017 This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The collaboration plans to build a staged 40 kt liquid argon detector at the Sanford Underground Research Facility in South Dakota, a high precision near detector, and a powerful neutrino beam line generated by a 1.2 MW proton beam produced by the PIP-II upgrade, evolving to a power of 2.3 MW by 2030. |
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ISSN: | 1687-7357 1687-7365 |
DOI: | 10.1155/2017/6590489 |