دورية أكاديمية

New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam

التفاصيل البيبلوغرافية
العنوان: New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam
المؤلفون: N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. Badertscher, A. Ben Dhahbi, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, G. Brunetti, B. Buttner, S. Buontempo, L. Chaussard, M. Chernyavskiy, V. Chiarella, A. Chukanov, L. Consiglio, N. D'Ambrosio, P. Amo Sanchez, G. Lellis, M. Serio, A. Crescenzo, D. Ferdinando, N. Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, J. Ebert, A. Ereditato, J. Favier, T. Ferber, R. A. Fini, T. Fukuda, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, A. M. Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, H. Kawahara, J. Kawada, J. H. Kim, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, P. Migliozzi, S. Mikado, A. Minotti, M. Miyanishi, E. Miyashita, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, T. Roganova, H. Rokujo, I. Rostovtseva, A. Rubbia, A. Russo, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt Parzefall, I. Shakiryanova, T. Schcedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, K. Suzuki, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, P. Tolun, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche, LOVERRE, Pier Ferruccio, ROSA, Giovanni
المساهمون: N., Agafonova, A., Aleksandrov, A., Anokhina, S., Aoki, A., Ariga, T., Ariga, T., Asada, D., Autiero, A., Badertscher, A., Ben Dhahbi, D., Bender, A., Bertolin, C., Bozza, R., Brugnera, G., Brunetti, B., Buttner, S., Buontempo, L., Chaussard, M., Chernyavskiy, V., Chiarella, A., Chukanov, L., Consiglio, N., D'Ambrosio, P., Amo Sanchez, G., Lelli, M., Serio, A., Crescenzo, D., Ferdinando, N., Marco, S., Dmitrievski, M., Draco, D., Duchesneau, S., Dusini, J., Ebert, A., Ereditato, J., Favier, T., Ferber, R. A., Fini, T., Fukuda, A., Garfagnini, G., Giacomelli, C., Goellnitz, J., Goldberg, Y., Gornushkin, G., Grella, F., Grianti, A. M., Guler, C., Gustavino, C., Hagner, K., Hakamata, T., Hara, T., Hayakawa, M., Hierholzer, A., Hollnagel, B., Hosseini, H., Ishida, K., Ishiguro, M., Ishikawa, K., Jakovcic, C., Jollet, C., Kamiscioglu, M., Kamiscioglu, T., Katsuragawa, H., Kawahara, J., Kawada, J. H., Kim, S. H., Kim, M., Kimura, N., Kitagawa, B., Klicek, K., Kodama, M., Komatsu, U., Kose, I., Kreslo, A., Lauria, J., Lenkeit, A., Ljubicic, A., Longhin, Loverre, Pier Ferruccio, A., Malgin, G., Mandrioli, J., Marteau, T., Matsuo, V., Matveev, N., Mauri, E., Medinaceli, A., Meregaglia, P., Migliozzi, S., Mikado, A., Minotti, M., Miyanishi, E., Miyashita, P., Monacelli, M. C., Montesi, K., Morishima, M. T., Muciaccia, N., Naganawa, T., Naka, M., Nakamura, T., Nakano
بيانات النشر: Springer Heidelberg
سنة النشر: 2013
المجموعة: Sapienza Università di Roma: CINECA IRIS
مصطلحات موضوعية: neutrino detectors and telescope, oscillation
الوصف: The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the νμ → ντ channel, via the detection of the τ-leptons created in charged current ντ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17GeV. The observation of the first ντ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ντ candidate has been observed. The significance of the two events in terms of a νμ → ντ oscillation signal is of 2.40σ.
نوع الوثيقة: article in journal/newspaper
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/wos/WOS:000326719900001; volume:2013; issue:11; journal:JOURNAL OF HIGH ENERGY PHYSICS; http://hdl.handle.net/11573/548156Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-84893056114
DOI: 10.1007/jhep11(2013)036
الإتاحة: https://doi.org/10.1007/jhep11Test(2013)036
http://hdl.handle.net/11573/548156Test
رقم الانضمام: edsbas.6A2500D4
قاعدة البيانات: BASE