1. Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
- Author
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G. De Lellis, S. Dmitrievsky, Kunihiro Morishima, B. D. Park, Chiara Sirignano, Caren Hagner, G. Galati, M. Miyanishi, S. Buontempo, F. Terranova, Nicola D'Ambrosio, N. Di Marco, A. M. Anokhina, Tatsuhiro Naka, Akitaka Ariga, A. S. Malgin, C. Gustavino, M. T. Muciaccia, Andrey Alexandrov, K. Niwa, Nobuko Kitagawa, Mitsuhiro Nakamura, R. Brugnera, P. Monacelli, N. Agafonova, M. Dracos, F. Laudisio, T. Hayakawa, Maria Cristina Montesi, Shigeki Aoki, Masahiro Komatsu, H. Rokujo, F. Fornari, M. Kamiscioglu, T. Shchedrina, T. Hara, D. A. Podgrudkov, S. Simone, Valeri Tioukov, J. L. Vuilleumier, Naotaka Naganawa, A. Buonaura, Pierre Vilain, G. Mandrioli, D. Di Ferdinando, Luca Stanco, A. Garfagnini, J. Goldberg, M. Chernyavskiy, B. Klicek, S. Mikado, M. Roda, Cécile Jollet, F. Pupilli, P. Strolin, Alessandro Paoloni, G. Grella, M. Tenti, J. Ebert, F. Mizutani, A. Sotnikov, Koichi Kodama, A. Hollnagel, T. M. Roganova, N. Mauri, C. Kamiscioglu, N. Okateva, H. Pessard, I. Shakiryanova, N. I. Starkov, Mario Stipčević, Lucia Votano, H. Shibuya, C. S. Yoon, A. Chukanov, Kazumi Ozaki, Natalia Polukhina, G. Rosa, M. Pozzato, L. Patrizii, Gaston Wilquet, D. Duchesneau, Seok Kim, Katsumi Ishiguro, M. De Serio, E. Voevodina, Tomoko Ariga, Timur Dzhatdoev, S. Vasina, Osamu Sato, Adele Lauria, A. Di Crescenzo, Krešimir Jakovčić, V. A. Matveev, Yuri Gornushkin, M. Spinetti, P. F. Loverre, L. Paparella, A. Iuliano, Simona Maria Stellacci, E. Shibayama, I. Kreslo, A. M. Guler, Utku Kose, P. del Amo Sanchez, O. Ryazhskaya, A. Pastore, T. Shiraishi, Satoru Takahashi, R. A. Fini, T. Fukuda, G. Sirri, Ante Ljubičić, A. Longhin, Anselmo Meregaglia, S. Ogawa, A. Schembri, T. Matsuo, Cristiano Bozza, V. Gentile, A. Ereditato, A. Bertolin, L. Pasqualini, E. Medinaceli, S. Dusini, L. Consiglio, S. Gorbunov, Toshiyuki Nakano, 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., Lellis G.D., Serio M.D., Sanchez P.D.A., Crescenzo A.D., Ferdinando D.D., Marco N.D., 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., Ljubicic 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., Paparella L., 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., Schembri A., Shakiryanova I., Shchedrina T., Shibayama E., Shibuya H., Shiraishi 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., Vasina S., Vilain P., Voevodina E., Votano L., Vuilleumier J.L., Wilquet G., Yoon C.S., Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), OPERA, Laboratoire d'Annecy de Physique des Particules (LAPP), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), 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., Lellis, G. De, Serio, M. De, Sanchez, P. del Amo, Crescenzo, A. Di, Ferdinando, D. Di, Marco, N. Di, 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., Jakovčić, K., Jollet, C., Kamiscioglu, C., Kamiscioglu, M., Kim, S. H., Kitagawa, N., Kliček, B., Kodama, K., Komatsu, M., Kose, U., Kreslo, I., Laudisio, F., Lauria, A., Ljubičić, 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., Paparella, L., 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., Schembri, A., Shakiryanova, I., Shchedrina, T., Shibayama, E., Shibuya, H., Shiraishi, T., Simone, S., Sirignano, C., Sirri, G., Sotnikov, A., Spinetti, M., Stanco, L., Starkov, N., Stellacci, S. M., Stipčević, M., Strolin, P., Takahashi, S., Tenti, M., Terranova, F., Tioukov, V., Vasina, S., Vilain, P., Voevodina, E., Votano, L., Vuilleumier, J. L., Wilquet, G., Yoon, C. S., 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, Lellis, G, Serio, M, Sanchez, P, Crescenzo, A, Ferdinando, D, Marco, N, Dmitrievsky, S, Dracos, M, Duchesneau, D, Dusini, S, Dzhatdoev, T, Ebert, J, Ereditato, A, Fini, R, Fornari, F, Fukuda, T, Galati, G, Garfagnini, A, Gentile, V, Goldberg, J, Gorbunov, S, Gornushkin, Y, Grella, G, Guler, A, Gustavino, C, Hagner, C, Hara, T, Hayakawa, T, Hollnagel, A, Ishiguro, K, Iuliano, A, Jakovcic, K, Jollet, C, Kamiscioglu, C, Kamiscioglu, M, Kim, S, Kitagawa, N, Klicek, B, Kodama, K, Komatsu, M, Kose, U, Kreslo, I, Laudisio, F, Lauria, A, Ljubicic, 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, Morishima, K, Muciaccia, M, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Niwa, K, Ogawa, S, Okateva, N, Ozaki, K, Paoloni, A, Paparella, L, Park, B, 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, Schembri, A, Shakiryanova, I, Shchedrina, T, Shibayama, E, Shibuya, H, Shiraishi, T, Simone, S, Sirignano, C, Sirri, G, Sotnikov, A, Spinetti, M, Stanco, L, Starkov, N, Stellacci, S, Stipcevic, M, Strolin, P, Takahashi, S, Tenti, M, Terranova, F, Tioukov, V, Vasina, S, Vilain, P, Voevodina, E, Votano, L, Vuilleumier, J, Wilquet, G, and Yoon, C
- Subjects
Physics - Instrumentation and Detectors ,cosmic rays detectors ,neutrino detectors ,neutrino experiments ,Physics::Instrumentation and Detectors ,01 natural sciences ,7. Clean energy ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,Physics::Popular Physics ,Observatory ,Tau neutrino ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,Nuclear emulsion ,Muon neutrino ,Detectors and Experimental Techniques ,Nuclear Experiment ,physics.ins-det ,Physics ,Detector ,OPERA ,Astrophysics::Instrumentation and Methods for Astrophysics ,resistive plate chamber ,Instrumentation and Detectors (physics.ins-det) ,observatory ,modulation ,nuclear emulsion ,neutrino detector ,neutrino/tau: particle identification ,Particle Physics - Experiment ,Particle physics ,atmosphere: temperature ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Cosmic ray ,Nuclear physics ,0103 physical sciences ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,cosmic rays detector ,muon: flux ,scintillation counter ,Muon ,hep-ex ,010308 nuclear & particles physics ,Astronomy and Astrophysics ,neutrino/mu: secondary beam ,Gran Sasso ,correlation ,muon: cosmic radiation ,High Energy Physics::Experiment ,neutrino: oscillation ,Lepton ,experimental results - Abstract
The OPERA experiment discovered muon neutrino into tau neutrino oscillations in appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus was also endowed with electronic detectors with tracking capability, such as scintillator strips and resistive plate chambers. Because of its location in the underground Gran Sasso laboratory, under 3800 m.w.e., the OPERA detector has also been used as an observatory for TeV muons produced by cosmic rays in the atmosphere. In this paper the measurement of the single muon flux modulation and its correlation with the seasonal cycle of atmospheric temperature is reported. The OPERA experiment discovered muon neutrino into tau neutrino oscillations in appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus was also endowed with electronic detectors with tracking capability, such as scintillator strips and resistive plate chambers. Because of its location, in the underground Gran Sasso laboratory, under 3800 m.w.e., the OPERA detector has also been used as an observatory for TeV muons produced by cosmic rays in the atmosphere. In this paper the measurement of the single muon flux modulation and of its correlation with the seasonal variation of the atmospheric temperature are reported.
- Published
- 2019
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