Detailed Information

Cited 6 time in webofscience Cited 6 time in scopus
Metadata Downloads

OPERA tau neutrino charged current interactionsopen access

Authors
Agafonova, N.Alexandrov, A.Anokhina, A.Aoki, S.Ariga, A.Ariga, T.Bertolin, A.Bozza, C.Brugnera, R.Buonaura, A.Buontempo, S.Chernyavskiy, M.Chukanov, A.Consiglio, L.D'Ambrosio, N.De Lellis, G.De Serio, M.del Amo Sanchez, P.Di Crescenzo, A.Di Ferdinando, D.Di Marco, N.Dmitrievsky, S.Dracos, M.Duchesneau, D.Dusini, S.Dzhatdoev, T.Ebert, J.Ereditato, A.Fini, R. A.Fornari, F.Fukuda, T.Galati, G.Garfagnini, A.Gentile, V.Goldberg, J.Gorbunov, S.Gornushkin, Y.Grella, G.Guler, A. M.Gustavino, C.Hagner, C.Hara, T.Hayakawa, T.Hollnagel, A.Ishiguro, K.Iuliano, A.Jakovcic, K.Jollet, C.Kamiscioglu, C.Kamiscioglu, M.Kim, S. H.Kitagawa, N.Klicek, B.Kodama, K.Komatsu, M.Kose, U.Kreslo, I.Laudisio, F.Lauria, A.Lavasa, A.Longhin, A.Loverre, P.Malgin, A.Mandrioli, G.Matsuo, T.Matveev, V.Mauri, N.Medinaceli, E.Meregaglia, A.Mikado, S.Miyanishi, M.Mizutani, F.Monacelli, P.Montesi, M. C.Morishima, K.Muciaccia, M. T.Naganawa, N.Naka, T.Nakamura, M.Nakano, T.Niwa, K.Ogawa, S.Okateva, N.Ozaki, K.Paoloni, A.Park, B. D.Pasqualini, L.Pastore, A.Patrizii, L.Pessard, H.Podgrudkov, D.Polukhina, N.Pozzato, M.Pupilli, F.Roda, M.Roganova, T.Rokujo, H.Rosa, G.Ryazhskaya, O.Sato, O.Shakirianova, I.Schembri, A.Shchedrina, T.Shibayama, E.Shibuya, H.Shiraishi, T.Simko, T.Simone, S.Sirignano, C.Sirri, G.Sotnikov, A.Spinetti, M.Stanco, L.Starkov, N.Stellacci, S. M.Stipcevic, M.Strolin, P.Takahashi, S.Tenti, M.Terranova, F.Tioukov, V.Tsanaktsidis, I.Tufanli, S.Ustyuzhanin, A.Vasina, S.Vidal Garcia, M.Vilain, P.Voevodina, E.Votano, L.Vuilleumier, J. L.Wilquet, G.Yoon, C. S.
Issue Date
Aug-2021
Publisher
NATURE PORTFOLIO
Citation
SCIENTIFIC DATA, v.8, no.1
Indexed
SCIE
SCOPUS
Journal Title
SCIENTIFIC DATA
Volume
8
Number
1
URI
https://scholarworks.gnu.ac.kr/handle/sw.gnu/72663
DOI
10.1038/s41597-021-00991-y
ISSN
2052-4463
Abstract
The OPERA experiment was designed to discover the v(tau) appearance in a v(mu) beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. It was exposed from 2008 to 2012 to the CNGS beam: an almost pure v(mu) beam with a baseline of 730 km, collecting a total of 1.8 center dot 10(20) protons on target. The OPERA Collaboration eventually assessed the discovery of v(mu)-> v(tau) oscillations with a statistical significance of 6.1 sigma by observing ten v(tau) CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a ydetailed description of the v(tau) data sample to make it usable by the whole community.
Files in This Item
There are no files associated with this item.
Appears in
Collections
ETC > Journal Articles

qrcode

Items in ScholarWorks are protected by copyright, with all rights reserved, unless otherwise indicated.

Altmetrics

Total Views & Downloads

BROWSE