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Deutsche Physikalische Gessellschaft IOP Institute of Physics

Study of neutrino interactions with the electronic detectors of the OPERA experiment

N Agafonova1, A Aleksandrov2, O Altinok3, A Anokhina4, S Aoki5, A Ariga6, T Ariga6, D Autiero7, A Badertscher8, A Bagulya9, A Bendhahbi10, A Bertolin11,39, C Bozza12, T Brugière7, R Brugnera11,13, F Brunet14, G Brunetti7,15,16, S Buontempo2, A Cazes7, L Chaussard7, M Chernyavskiy9, V Chiarella17, A Chukanov18, N D'Ambrosio19, F Dal Corso11, G De Lellis2,20, P del Amo Sanchez14, Y Déclais7, M De Serio21, F Di Capua2, A Di Crescenzo2,20, D Di Ferdinando16, N Di Marco22,40, S Dmitrievski18, M Dracos23, D Duchesneau14, S Dusini11, T Dzhatdoev4, J Ebert24, O Egorov25, R Enikeev1, A Ereditato6, L S Esposito8, J Favier14, T Ferber24, R A Fini21, D Frekers26, T Fukuda27, A Garfagnini11,13, G Giacomelli15,16, M Giorgini15,16,41, C Göllnitz24, J Goldberg28, D Golubkov25, L Goncharova9, Y Gornushkin18, G Grella12, F Grianti17,29, A M Guler3, C Gustavino19,42, C Hagner24, K Hamada27, T Hara5, M Hierholzer24, A Hollnagel24, K Hoshino27, M Ieva21, H Ishida30, K Jakovcic31, C Jollet23,47, F Juget6, M Kamiscioglu3, K Kazuyama27, S H Kim32,43, M Kimura30, N Kitagawa27, B Klicek31, J Knuesel6, K Kodama33, M Komatsu27, U Kose11,13, I Kreslo6, H Kubota27, C Lazzaro8, J Lenkeit24, I Lippi11, A Ljubicic31, A Longhin11,13,44, P Loverre34, G Lutter6, A Malgin1, G Mandrioli16, K Mannai10, J Marteau7, T Matsuo30, V Matveev1, N Mauri15,16,43, E Medinaceli16, F Meisel6, A Meregaglia23,47, P Migliozzi2, S Mikado30, S Miyamoto27, P Monacelli22, K Morishima27, U Moser6, M T Muciaccia21,35, N Naganawa27, T Naka27, M Nakamura27, T Nakano27, D Naumov18, V Nikitina4, K Niwa27, Y Nonoyama27, S Ogawa30, N Okateva9, A Olchevskiy18, M Paniccia17, A Paoloni17, B D Park32,45, I G Park32, A Pastore21,35, L Patrizii16, E Pennacchio7, H Pessard14, K Pretzl6, V Pilipenko26, C Pistillo6, N Polukhina9, M Pozzato15,16, F Pupilli22, R Rescigno12, T Roganova4, H Rokujo5, G Romano12, G Rosa34, I Rostovtseva25, A Rubbia8, A Russo2, V Ryasny1, O Ryazhskaya1, O Sato27, Y Sato36, A Schembri19, W Schmidt-Parzefall24, H Schroeder37, L Scotto Lavina2,20,46, A Sheshukov18, H Shibuya30, G Shoziyeov4, S Simone21,35, M Sioli15,16, C Sirignano12, G Sirri16, J S Song32, M Spinetti17, L Stanco11, N Starkov9, M Stipcevic31, T Strauss8,47, P Strolin2,20, S Takahashi27, M Tenti15,16, F Terranova17, I Tezuka36, V Tioukov2, P Tolun3, A Trabelsi10, T Tran7, S Tufanli3,46, P Vilain38, M Vladimirov9, L Votano17, J L Vuilleumier6, G Wilquet28, B Wonsak24, V Yakushev1, C S Yoon32, T Yoshioka27, J Yoshida27, Y Zaitsev25, S Zemskova18, A Zghiche14 and R Zimmermann24

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The OPERA experiment is based on a hybrid technology combining electronic detectors (EDs) and nuclear emulsions. OPERA collected muon–neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an energy range of about 5–35 GeV. A total of 5.3×1019 protons on target equivalent luminosity have been analysed with the OPERA EDs: scintillator strips target trackers and magnetic muon spectrometers equipped with resistive plate gas chambers and drift tubes, allowing a detailed reconstruction of muon–neutrino interactions. Charged current (CC) and neutral current (NC) interactions are identified, using the measurements in the EDs, and the NC/CC ratio is computed. The momentum distribution and the charge of the muon tracks produced in CC interactions are analysed. Calorimetric measurements of the visible energy are performed for both the CC and NC samples. For CC events, the Bjorken-y distribution and the hadronic shower profile are computed. The results are compared with a detailed Monte Carlo simulation of the response of EDs.


PACS

29.40.Rg Nuclear emulsions

12.15.Mm Neutral currents

29.50.+v Computer interfaces

29.40.Mc Scintillation detectors

29.40.Vj Calorimeters

Subjects

Accelerators, beams and electromagnetism

Nuclear physics

Instrumentation and measurement

Particle physics and field theory

Dates

Issue 5 (May 2011)

Received 10 February 2011

Published 26 May 2011



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