Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector

被引：12

作者：

Agafonova, N. ^{[1
]}

Alexandrov, A. ^{[2
]}

Anokhina, A. ^{[3
]}

Aoki, S. ^{[4
]}

Ariga, A. ^{[5
]}

Ariga, T. ^{[5
,6
]}

Bertolin, A. ^{[7
]}

Bozza, C. ^{[8
,9
]}

Brugnera, R. ^{[7
,10
]}

Buonaura, A. ^{[2
,11
,38
]}

Buontempo, S. ^{[2
]}

Chernyavskiy, M. ^{[12
]}

Chukanov, A. ^{[13
]}

Consiglio, L. ^{[2
]}

D'Ambrosio, N. ^{[14
]}

De Lellis, G. ^{[2
,11
]}

De Serio, M. ^{[15
,16
]}

Sanchez, P. del Amo ^{[17
]}

Di Crescenzo, A. ^{[2
,11
]}

Di Ferdinando, D. ^{[18
]}

Di Marco, N. ^{[14
]}

Dmitrievsky, S. ^{[13
]}

Dracos, M. ^{[19
]}

Duchesneau, D. ^{[17
]}

Dusini, S. ^{[7
]}

Dzhatdoev, T. ^{[3
]}

Ebert, J. ^{[20
]}

Ereditato, A. ^{[5
]}

Fini, R. A. ^{[16
]}

Fornari, F. ^{[18
,21
]}

Fukuda, T. ^{[22
]}

Galati, G. ^{[2
,11
]}

Garfagnini, A. ^{[7
,10
]}

Gentile, V ^{[23
]}

Goldberg, J. ^{[24
]}

Gorbunov, S. ^{[12
]}

Gornushkin, Y. ^{[13
]}

Grella, G. ^{[8
,9
]}

Guler, A. M. ^{[25
]}

Gustavino, C. ^{[26
]}

Hagner, C. ^{[20
]}

Hara, T. ^{[4
]}

Hayakawa, T. ^{[22
]}

Hollnagel, A. ^{[20
]}

Ishiguro, K. ^{[22
]}

Iuliano, A. ^{[2
,11
]}

Jakovcic, K. ^{[28
]}

Jollet, C. ^{[19
]}

Kamiscioglu, C. ^{[25
,29
]}

Kamiscioglu, M. ^{[25
]}

机构：

[1] Russian Acad Sci, Inst Nucl Res, RUS-117312 Moscow, Russia

[2] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

[3] Lomonosov Moscow State Univ, SINP MSU Skobeltsyn Inst Nucl Phys, RUS-119991 Moscow, Russia

[4] Kobe Univ, Kobe, Hyogo 6578501, Japan

[5] Univ Bern, Albert Einstein Ctr Fundamental Phys, LHEP, CH-3012 Bern, Switzerland

[6] Kyushu Univ, Fac Arts & Sci, Fukuoka, Fukuoka 8190395, Japan

[7] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[8] Univ Salerno, Dipartimento Fis, I-84084 Salerno, Italy

[9] Ist Nazl Fis Nucl, Grp Collegato, I-84084 Salerno, Italy

[10] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy

[11] Univ Federico II Napoli, Dipartimento Fis, I-80126 Naples, Italy

[12] Russian Acad Sci, LPI, RUS-119991 Moscow, Russia

[13] Joint Inst Nucl Res, RUS-141980 Dubna, Russia

[14] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Laquila, Italy

[15] Univ Bari, Dipartimento Fis, I-70126 Bari, Italy

[16] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[17] Univ Savoie Mt Blanc, CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France

[18] Ist Nazl Fis Nucl, Sez Bologna, I-40127 Bologna, Italy

[19] Univ Strasbourg, CNRS, IN2P3, IPHC, F-67037 Strasbourg, France

[20] Hamburg Univ, D-22761 Hamburg, Germany

[21] Univ Bologna, Dipartimento Fis & Astron, I-40127 Bologna, Italy

[22] Nagoya Univ, Nagoya, Aichi 4648602, Japan

[23] GSSI, I-40127 Laquila, Italy

[24] Technion, Dept Phys, IL-32000 Haifa, Israel

[25] Middle East Tech Univ, TR-06800 Ankara, Turkey

[26] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[27] Univ Libre Bruxelles, IIHE, B-1050 Brussels, Belgium

[28] Rudjer Boskovic Inst, HR-10000 Zagreb, Croatia

[29] Ankara Univ, TR-06560 Ankara, Turkey

[30] Gyeongsang Natl Univ, 900 Gazwa Dong, Jinju 660701, South Korea

[31] Rudjer Boskovic Inst, Ctr Excellence Adv Mat & Sensing, HR-10000 Zagreb, Croatia

[32] Aichi Univ Educ, Kariya, Aichi 4488542, Japan

[33] Toho Univ, Funabashi, Chiba 2748510, Japan

[34] Nihon Univ, Narashino, Chiba 2758576, Japan

[35] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Rome, Italy

[36] MEPhI Moscow Engn Phys Inst, RUS-115409 Moscow, Russia

[37] Univ Milano Bicocca, Dipartimento Fis, I-20126 Milan, Italy

[38] Univ Zurich, Phys Inst, Zurich, Switzerland

[39] CERN, Geneva, Switzerland

[40] Osserv Astron Padova, Padua, Italy

[41] Univ Liverpool, Liverpool, Merseyside, England

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2019年 / 10期

基金：

新加坡国家研究基金会; 俄罗斯基础研究基金会;

关键词：

cosmic rays detectors; neutrino detectors; neutrino experiments;

D O I：

10.1088/1475-7516/2019/10/003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：15

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