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OPERA tau neutrino charged current interactions.


ABSTRACT: The OPERA experiment was designed to discover the vτ appearance in a vμ 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 vμ beam with a baseline of 730 km, collecting a total of 1.8·1020 protons on target. The OPERA Collaboration eventually assessed the discovery of vμ→vτ oscillations with a statistical significance of 6.1 σ by observing ten vτ CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a detailed description of the vτ data sample to make it usable by the whole community.

SUBMITTER: Agafonova N 

PROVIDER: S-EPMC8361145 | biostudies-literature | 2021 Aug

REPOSITORIES: biostudies-literature

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OPERA tau neutrino charged current interactions.

Agafonova N N   Alexandrov A A   Anokhina A A   Aoki S S   Ariga A A   Ariga T T   Bertolin A A   Bozza C C   Brugnera R R   Buonaura A A   Buontempo S S   Chernyavskiy M M   Chukanov A A   Consiglio L L   D'Ambrosio N N   De Lellis G G   De Serio M M   Del Amo Sanchez P P   Di Crescenzo A A   Di Ferdinando D D   Di Marco N N   Dmitrievsky S S   Dracos M M   Duchesneau D D   Dusini S S   Dzhatdoev T T   Ebert J J   Ereditato A A   Fini R A RA   Fornari F F   Fukuda T T   Galati G G   Garfagnini A A   Gentile V V   Goldberg J J   Gorbunov S S   Gornushkin Y Y   Grella G G   Guler A M AM   Gustavino C C   Hagner C C   Hara T T   Hayakawa T T   Hollnagel A A   Ishiguro K K   Iuliano A A   Jakovčić K K   Jollet C C   Kamiscioglu C C   Kamiscioglu M M   Kim S H SH   Kitagawa N N   Kliček B B   Kodama K K   Komatsu M M   Kose U U   Kreslo I I   Laudisio F F   Lauria A A   Lavasa A A   Longhin A A   Loverre P P   Malgin A A   Mandrioli G G   Matsuo T T   Matveev V V   Mauri N N   Medinaceli E E   Meregaglia A A   Mikado S S   Miyanishi M M   Mizutani F F   Monacelli P P   Montesi M C MC   Morishima K K   Muciaccia M T MT   Naganawa N N   Naka T T   Nakamura M M   Nakano T T   Niwa K K   Ogawa S S   Okateva N N   Ozaki K K   Paoloni A A   Park B D BD   Pasqualini L L   Pastore A A   Patrizii L L   Pessard H H   Podgrudkov D D   Polukhina N N   Pozzato M M   Pupilli F F   Roda M M   Roganova T T   Rokujo H H   Rosa G G   Ryazhskaya O O   Sato O O   Shakirianova I I   Schembri A A   Shchedrina T T   Shibayama E E   Shibuya H H   Shiraishi T T   Šimko T T   Simone S S   Sirignano C C   Sirri G G   Sotnikov A A   Spinetti M M   Stanco L L   Starkov N N   Stellacci S M SM   Stipčević M M   Strolin P P   Takahashi S S   Tenti M M   Terranova F F   Tioukov V V   Tsanaktsidis I I   Tufanli S S   Ustyuzhanin A A   Vasina S S   Vidal García M M   Vilain P P   Voevodina E E   Votano L L   Vuilleumier J L JL   Wilquet G G   Yoon C S CS  

Scientific data 20210812 1


The OPERA experiment was designed to discover the v<sub>τ</sub> appearance in a v<sub>μ</sub> 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<sub>μ</sub> beam with a baseline of 730 km, collecting a total of 1.8·10<sup>20</sup> protons on target. The OPER  ...[more]

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