Measurement of the atmospheric muon charge ratio with the OPERA detector

N. Agafonova; A. Anokhina; S. Aoki; A. Ariga; T. Ariga; D. Autiero; A. Badertscher; A. Bagulya; A. Bertolin; M. Besnier; D. Bick; V. Boyarkin; C. Bozza; T. Brugière; R. Brugnera; G. Brunetti; S. Buontempo; A. Cazes; L. Chaussard; M. Chernyavsky; V. Chiarella; N. Chon-Sen; A. Chukanov; M. Cozzi; G. D'Amato; F. Dal Corso; N. D'Ambrosio; G. De Lellis; Y. Déclais; M. De Serio; F. Di Capua; D. Di Ferdinando; A. Di Giovanni; N. Di Marco; S. Dmitrievski; M. Dracos; D. Duchesneau; S. Dusini; J. Ebert; O. Egorov; R. Enikeev; A. Ereditato; L. S. Esposito; J. Favier; G. Felici; T. Ferber; R. Fini; D. Frekers; T. Fukuda; C. Fukushima; V. I. Galkin; A. Garfagnini; G. Giacomelli; M. Giorgini; C. Goellnitz; J. Goldberg; D. Golubkov; L. Goncharova; Y. Gornushkin; G. Grella; F. Grianti; M. Guler; C. Gustavino; C. Hagner; K. Hamada; T. Hara; M. Hierholzer; K. Hoshino; M. Ieva; K. Jakovcic; C. Jollet; F. Juget; M. Kazuyama; S. H. Kim; M. Kimura; B. Klicek; J. Knuesel; K. Kodama; M. Komatsu; U. Kose; I. Kreslo; H. Kubota; C. Lazzaro; J. Lenkeit; A. Ljubicic; A. Longhin; G. Lutter; A. Malgin; G. Mandrioli; A. Marotta; J. Marteau; T. Matsuo; V. Matveev; N. Mauri; E. Medinaceli; F. Meisel; A. Meregaglia; P. Migliozzi; S. Mikado; S. Miyamoto; P. Monacelli; K. Morishima; U. Moser; M. T. Muciaccia; N. Naganawa; T. Naka; M. Nakamura; T. Nakano; D. Naumov; V. Nikitina; K. Niwa; Y. Nonoyama; S. Ogawa; A. Olchevski; C. Oldorf; G. Orlova; V. Osedlo; M. Paniccia; A. Paoloni; B. D. Park; I. G. Park; A. Pastore; L. Patrizii; E. Pennacchio; H. Pessard; V. Pilipenko; C. Pistillo; G. Policastro; N. Polukhina; M. Pozzato; K. Pretzl; P. Publichenko; F. Pupilli; R. Rescigno; T. Roganova; H. Rokujo; G. Romano; G. Rosa; I. Rostovtseva; A. Rubbia; A. Russo; V. Ryasny; O. Ryazhskaya; O. Sato; Y. Sato; A. Schembri; W. Schmidt Parzefall; H. Schroeder; L. Scotto Lavina; A. Sheshukov; H. Shibuya; S. Simone; M. Sioli; C. Sirignano; G. Sirri; J. S. Song; M. Spinetti; L. Stanco; N. Starkov; M. Stipcevic; T. Strauss; P. Strolin; S. Takahashi; M. Tenti; F. Terranova; I. Tezuka; V. Tioukov; P. Tolun; T. Tran; S. Tufanli; P. Vilain; M. Vladimirov; L. Votano; J. L. Vuilleumier; G. Wilquet; B. Wonsak; V. Yakushev; C. S. Yoon; T. Yoshioka; J. Yoshida; Y. Zaitsev; S. Zemskova; A. Zghiche; R. Zimmermann

doi:10.1140/epjc/s10052-010-1284-8

Measurement of the atmospheric muon charge ratio with the OPERA detector

N. Agafonova
, A. Anokhina
, S. Aoki
, A. Ariga
, T. Ariga
, D. Autiero
, A. Badertscher
, A. Bagulya
, A. Bertolin
, M. Besnier
, D. Bick
, V. Boyarkin
, C. Bozza
, T. Brugière
, R. Brugnera
, G. Brunetti
, S. Buontempo
, A. Cazes
, L. Chaussard
, M. Chernyavsky

V. Chiarella, N. Chon-Sen, A. Chukanov, M. Cozzi, G. D'Amato, F. Dal Corso, N. D'Ambrosio, G. De Lellis, Y. Déclais, M. De Serio, F. Di Capua, D. Di Ferdinando, A. Di Giovanni, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, J. Ebert, O. Egorov, R. Enikeev, A. Ereditato, L. S. Esposito, J. Favier, G. Felici, T. Ferber, R. Fini, D. Frekers, T. Fukuda, C. Fukushima, V. I. Galkin, A. Garfagnini, G. Giacomelli, M. Giorgini, C. Goellnitz, J. Goldberg, D. Golubkov, L. Goncharova, Y. Gornushkin, G. Grella, F. Grianti, M. Guler, C. Gustavino, C. Hagner, K. Hamada, T. Hara, M. Hierholzer, K. Hoshino, M. Ieva, K. Jakovcic, C. Jollet, F. Juget, M. Kazuyama, S. H. Kim, M. Kimura, B. Klicek, J. Knuesel, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, H. Kubota, C. Lazzaro, J. Lenkeit, A. Ljubicic, A. Longhin, G. Lutter, A. Malgin, G. Mandrioli, A. Marotta, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, F. Meisel, A. Meregaglia, P. Migliozzi, S. Mikado, S. Miyamoto, P. Monacelli, K. Morishima, U. Moser, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, D. Naumov, V. Nikitina, K. Niwa, Y. Nonoyama, S. Ogawa, A. Olchevski, C. Oldorf, G. Orlova, V. Osedlo, M. Paniccia, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, V. Pilipenko, C. Pistillo, G. Policastro, N. Polukhina, M. Pozzato, K. Pretzl, P. Publichenko, F. Pupilli, R. Rescigno, T. Roganova, H. Rokujo, G. Romano, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, V. Ryasny, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt Parzefall, H. Schroeder, L. Scotto Lavina, A. Sheshukov, H. Shibuya, S. Simone, M. Sioli, C. Sirignano, G. Sirri, J. S. Song, M. Spinetti, L. Stanco, N. Starkov, M. Stipcevic, T. Strauss, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, I. Tezuka, V. Tioukov, P. Tolun, T. Tran, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, V. Yakushev, C. S. Yoon, T. Yoshioka, J. Yoshida, Y. Zaitsev, S. Zemskova, A. Zghiche, R. Zimmermann

Institute for Nuclear Research of the Russian Academy of Sciences
Moscow State University
Kobe University
University of Bern
IGFL, Université de Lyon, Université Lyon 1
ETH Zurich
P.N. Lebedev Physical Institute of the Russian Academy of Sciences
INFN
Université Savoie Mont Blanc
Universität Hamburg
University of Salerno
University of Padova
University of Bologna
INFN Sezione di Bologna
INFN Sezione di Napoli
LNF-INFN
Université de Strasbourg
Laboratori Nazionali del Gran Sasso
University of Naples Federico II
INFN Sezione di Bari
Università Dell'Aquila
Joint Institute for Nuclear Research, Dubna
Institute for Theoretical and Experimental Physics
University of Münster
Nagoya University
Toho University
Technion - Israel Institute of Technology
Middle East Technical University (METU)
Universität Rostock
Ruđer Bošković Institute
Gyeongsang National University
Aichi University of Education
Università degli studi di Bari Aldo Moro
Dipartimento di Fisica
Utsunomiya University
Université Libre de Bruxelles

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

41 Citations (Scopus)

Résumé

The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. We computed separately the muon charge ratio for single and for multiple muon events in order to select different energy regions of the primary cosmic ray spectrum and to test the R_μ dependence on the primary composition. The measured R_μ values were corrected taking into account the charge-misidentification errors. Data have also been grouped in five bins of the "vertical surface energy" ℰ_μcos θ. A fit to a simplified model of muon production in the atmosphere allowed the determination of the pion and kaon charge ratios weighted by the cosmic ray energy spectrum.

langue originale	Anglais
Pages (de - à)	25-37
Nombre de pages	13
journal	European Physical Journal C
Volume	67
Numéro de publication	1
Les DOIs	https://doi.org/10.1140/epjc/s10052-010-1284-8
état	Publié - 1 mai 2010
Modification externe	Oui

Accès au document

10.1140/epjc/s10052-010-1284-8

Contient cette citation

Agafonova, N., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Autiero, D., Badertscher, A., Bagulya, A., Bertolin, A., Besnier, M., Bick, D., Boyarkin, V., Bozza, C., Brugière, T., Brugnera, R., Brunetti, G., Buontempo, S., Cazes, A., Chaussard, L., ... Zimmermann, R. (2010). Measurement of the atmospheric muon charge ratio with the OPERA detector. European Physical Journal C, 67(1), 25-37. https://doi.org/10.1140/epjc/s10052-010-1284-8

@article{08bcbd55519746a0807bbd793ce76cb1,

title = "Measurement of the atmospheric muon charge ratio with the OPERA detector",

abstract = "The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. We computed separately the muon charge ratio for single and for multiple muon events in order to select different energy regions of the primary cosmic ray spectrum and to test the Rμ dependence on the primary composition. The measured Rμ values were corrected taking into account the charge-misidentification errors. Data have also been grouped in five bins of the {"}vertical surface energy{"} ℰμcos θ. A fit to a simplified model of muon production in the atmosphere allowed the determination of the pion and kaon charge ratios weighted by the cosmic ray energy spectrum.",

author = "N. Agafonova and A. Anokhina and S. Aoki and A. Ariga and T. Ariga and D. Autiero and A. Badertscher and A. Bagulya and A. Bertolin and M. Besnier and D. Bick and V. Boyarkin and C. Bozza and T. Brugi{\`e}re and R. Brugnera and G. Brunetti and S. Buontempo and A. Cazes and L. Chaussard and M. Chernyavsky and V. Chiarella and N. Chon-Sen and A. Chukanov and M. Cozzi and G. D'Amato and \{Dal Corso\}, F. and N. D'Ambrosio and \{De Lellis\}, G. and Y. D{\'e}clais and \{De Serio\}, M. and \{Di Capua\}, F. and \{Di Ferdinando\}, D. and \{Di Giovanni\}, A. and \{Di Marco\}, N. and S. Dmitrievski and M. Dracos and D. Duchesneau and S. Dusini and J. Ebert and O. Egorov and R. Enikeev and A. Ereditato and Esposito, \{L. S.\} and J. Favier and G. Felici and T. Ferber and R. Fini and D. Frekers and T. Fukuda and C. Fukushima and Galkin, \{V. I.\} and A. Garfagnini and G. Giacomelli and M. Giorgini and C. Goellnitz and J. Goldberg and D. Golubkov and L. Goncharova and Y. Gornushkin and G. Grella and F. Grianti and M. Guler and C. Gustavino and C. Hagner and K. Hamada and T. Hara and M. Hierholzer and K. Hoshino and M. Ieva and K. Jakovcic and C. Jollet and F. Juget and M. Kazuyama and Kim, \{S. H.\} and M. Kimura and B. Klicek and J. Knuesel and K. Kodama and M. Komatsu and U. Kose and I. Kreslo and H. Kubota and C. Lazzaro and J. Lenkeit and A. Ljubicic and A. Longhin and G. Lutter and A. Malgin and G. Mandrioli and A. Marotta and J. Marteau and T. Matsuo and V. Matveev and N. Mauri and E. Medinaceli and F. Meisel and A. Meregaglia and P. Migliozzi and S. Mikado and S. Miyamoto and P. Monacelli and K. Morishima and U. Moser and Muciaccia, \{M. T.\} and N. Naganawa and T. Naka and M. Nakamura and T. Nakano and D. Naumov and V. Nikitina and K. Niwa and Y. Nonoyama and S. Ogawa and A. Olchevski and C. Oldorf and G. Orlova and V. Osedlo and M. Paniccia and A. Paoloni and Park, \{B. D.\} and Park, \{I. G.\} and A. Pastore and L. Patrizii and E. Pennacchio and H. Pessard and V. Pilipenko and C. Pistillo and G. Policastro and N. Polukhina and M. Pozzato and K. Pretzl and P. Publichenko and F. Pupilli and R. Rescigno and T. Roganova and H. Rokujo and G. Romano and G. Rosa and I. Rostovtseva and A. Rubbia and A. Russo and V. Ryasny and O. Ryazhskaya and O. Sato and Y. Sato and A. Schembri and \{Schmidt Parzefall\}, W. and H. Schroeder and \{Scotto Lavina\}, L. and A. Sheshukov and H. Shibuya and S. Simone and M. Sioli and C. Sirignano and G. Sirri and Song, \{J. S.\} and M. Spinetti and L. Stanco and N. Starkov and M. Stipcevic and T. Strauss and P. Strolin and S. Takahashi and M. Tenti and F. Terranova and I. Tezuka and V. Tioukov and P. Tolun and T. Tran and S. Tufanli and P. Vilain and M. Vladimirov and L. Votano and Vuilleumier, \{J. L.\} and G. Wilquet and B. Wonsak and V. Yakushev and Yoon, \{C. S.\} and T. Yoshioka and J. Yoshida and Y. Zaitsev and S. Zemskova and A. Zghiche and R. Zimmermann",

year = "2010",

month = may,

day = "1",

doi = "10.1140/epjc/s10052-010-1284-8",

language = "English",

volume = "67",

pages = "25--37",

journal = "European Physical Journal C",

issn = "1434-6044",

publisher = "Springer Nature",

number = "1",

}

Agafonova, N, Anokhina, A, Aoki, S, Ariga, A, Ariga, T, Autiero, D, Badertscher, A, Bagulya, A, Bertolin, A, Besnier, M, Bick, D, Boyarkin, V, Bozza, C, Brugière, T, Brugnera, R, Brunetti, G, Buontempo, S, Cazes, A, Chaussard, L, Chernyavsky, M, Chiarella, V, Chon-Sen, N, Chukanov, A, Cozzi, M, D'Amato, G, Dal Corso, F, D'Ambrosio, N, De Lellis, G, Déclais, Y, De Serio, M, Di Capua, F, Di Ferdinando, D, Di Giovanni, A, Di Marco, N, Dmitrievski, S, Dracos, M, Duchesneau, D, Dusini, S, Ebert, J, Egorov, O, Enikeev, R, Ereditato, A, Esposito, LS, Favier, J, Felici, G, Ferber, T, Fini, R, Frekers, D, Fukuda, T, Fukushima, C, Galkin, VI, Garfagnini, A, Giacomelli, G, Giorgini, M, Goellnitz, C, Goldberg, J, Golubkov, D, Goncharova, L, Gornushkin, Y, Grella, G, Grianti, F, Guler, M, Gustavino, C, Hagner, C, Hamada, K, Hara, T, Hierholzer, M, Hoshino, K, Ieva, M, Jakovcic, K, Jollet, C, Juget, F, Kazuyama, M, Kim, SH, Kimura, M, Klicek, B, Knuesel, J, Kodama, K, Komatsu, M, Kose, U, Kreslo, I, Kubota, H, Lazzaro, C, Lenkeit, J, Ljubicic, A, Longhin, A, Lutter, G, Malgin, A, Mandrioli, G, Marotta, A, Marteau, J, Matsuo, T, Matveev, V, Mauri, N, Medinaceli, E, Meisel, F, Meregaglia, A, Migliozzi, P, Mikado, S, Miyamoto, S, Monacelli, P, Morishima, K, Moser, U, Muciaccia, MT, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Naumov, D, Nikitina, V, Niwa, K, Nonoyama, Y, Ogawa, S, Olchevski, A, Oldorf, C, Orlova, G, Osedlo, V, Paniccia, M, Paoloni, A, Park, BD, Park, IG, Pastore, A, Patrizii, L, Pennacchio, E, Pessard, H, Pilipenko, V, Pistillo, C, Policastro, G, Polukhina, N, Pozzato, M, Pretzl, K, Publichenko, P, Pupilli, F, Rescigno, R, Roganova, T, Rokujo, H, Romano, G, Rosa, G, Rostovtseva, I, Rubbia, A, Russo, A, Ryasny, V, Ryazhskaya, O, Sato, O, Sato, Y, Schembri, A, Schmidt Parzefall, W, Schroeder, H, Scotto Lavina, L, Sheshukov, A, Shibuya, H, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Song, JS, Spinetti, M, Stanco, L, Starkov, N, Stipcevic, M, Strauss, T, Strolin, P, Takahashi, S, Tenti, M, Terranova, F, Tezuka, I, Tioukov, V, Tolun, P, Tran, T, Tufanli, S, Vilain, P, Vladimirov, M, Votano, L, Vuilleumier, JL, Wilquet, G, Wonsak, B, Yakushev, V, Yoon, CS, Yoshioka, T, Yoshida, J, Zaitsev, Y, Zemskova, S, Zghiche, A & Zimmermann, R 2010, 'Measurement of the atmospheric muon charge ratio with the OPERA detector', European Physical Journal C, VOL. 67, Numéro 1, p. 25-37. https://doi.org/10.1140/epjc/s10052-010-1284-8

TY - JOUR

T1 - Measurement of the atmospheric muon charge ratio with the OPERA detector

AU - Agafonova, N.

AU - Anokhina, A.

AU - Aoki, S.

AU - Ariga, A.

AU - Ariga, T.

AU - Autiero, D.

AU - Badertscher, A.

AU - Bagulya, A.

AU - Bertolin, A.

AU - Besnier, M.

AU - Bick, D.

AU - Boyarkin, V.

AU - Bozza, C.

AU - Brugière, T.

AU - Brugnera, R.

AU - Brunetti, G.

AU - Buontempo, S.

AU - Cazes, A.

AU - Chaussard, L.

AU - Chernyavsky, M.

AU - Chiarella, V.

AU - Chon-Sen, N.

AU - Chukanov, A.

AU - Cozzi, M.

AU - D'Amato, G.

AU - Dal Corso, F.

AU - D'Ambrosio, N.

AU - De Lellis, G.

AU - Déclais, Y.

AU - De Serio, M.

AU - Di Capua, F.

AU - Di Ferdinando, D.

AU - Di Giovanni, A.

AU - Di Marco, N.

AU - Dmitrievski, S.

AU - Dracos, M.

AU - Duchesneau, D.

AU - Dusini, S.

AU - Ebert, J.

AU - Egorov, O.

AU - Enikeev, R.

AU - Ereditato, A.

AU - Esposito, L. S.

AU - Favier, J.

AU - Felici, G.

AU - Ferber, T.

AU - Fini, R.

AU - Frekers, D.

AU - Fukuda, T.

AU - Fukushima, C.

AU - Galkin, V. I.

AU - Garfagnini, A.

AU - Giacomelli, G.

AU - Giorgini, M.

AU - Goellnitz, C.

AU - Goldberg, J.

AU - Golubkov, D.

AU - Goncharova, L.

AU - Gornushkin, Y.

AU - Grella, G.

AU - Grianti, F.

AU - Guler, M.

AU - Gustavino, C.

AU - Hagner, C.

AU - Hamada, K.

AU - Hara, T.

AU - Hierholzer, M.

AU - Hoshino, K.

AU - Ieva, M.

AU - Jakovcic, K.

AU - Jollet, C.

AU - Juget, F.

AU - Kazuyama, M.

AU - Kim, S. H.

AU - Kimura, M.

AU - Klicek, B.

AU - Knuesel, J.

AU - Kodama, K.

AU - Komatsu, M.

AU - Kose, U.

AU - Kreslo, I.

AU - Kubota, H.

AU - Lazzaro, C.

AU - Lenkeit, J.

AU - Ljubicic, A.

AU - Longhin, A.

AU - Lutter, G.

AU - Malgin, A.

AU - Mandrioli, G.

AU - Marotta, A.

AU - Marteau, J.

AU - Matsuo, T.

AU - Matveev, V.

AU - Mauri, N.

AU - Medinaceli, E.

AU - Meisel, F.

AU - Meregaglia, A.

AU - Migliozzi, P.

AU - Mikado, S.

AU - Miyamoto, S.

AU - Monacelli, P.

AU - Morishima, K.

AU - Moser, U.

AU - Muciaccia, M. T.

AU - Naganawa, N.

AU - Naka, T.

AU - Nakamura, M.

AU - Nakano, T.

AU - Naumov, D.

AU - Nikitina, V.

AU - Niwa, K.

AU - Nonoyama, Y.

AU - Ogawa, S.

AU - Olchevski, A.

AU - Oldorf, C.

AU - Orlova, G.

AU - Osedlo, V.

AU - Paniccia, M.

AU - Paoloni, A.

AU - Park, B. D.

AU - Park, I. G.

AU - Pastore, A.

AU - Patrizii, L.

AU - Pennacchio, E.

AU - Pessard, H.

AU - Pilipenko, V.

AU - Pistillo, C.

AU - Policastro, G.

AU - Polukhina, N.

AU - Pozzato, M.

AU - Pretzl, K.

AU - Publichenko, P.

AU - Pupilli, F.

AU - Rescigno, R.

AU - Roganova, T.

AU - Rokujo, H.

AU - Romano, G.

AU - Rosa, G.

AU - Rostovtseva, I.

AU - Rubbia, A.

AU - Russo, A.

AU - Ryasny, V.

AU - Ryazhskaya, O.

AU - Sato, O.

AU - Sato, Y.

AU - Schembri, A.

AU - Schmidt Parzefall, W.

AU - Schroeder, H.

AU - Scotto Lavina, L.

AU - Sheshukov, A.

AU - Shibuya, H.

AU - Simone, S.

AU - Sioli, M.

AU - Sirignano, C.

AU - Sirri, G.

AU - Song, J. S.

AU - Spinetti, M.

AU - Stanco, L.

AU - Starkov, N.

AU - Stipcevic, M.

AU - Strauss, T.

AU - Strolin, P.

AU - Takahashi, S.

AU - Tenti, M.

AU - Terranova, F.

AU - Tezuka, I.

AU - Tioukov, V.

AU - Tolun, P.

AU - Tran, T.

AU - Tufanli, S.

AU - Vilain, P.

AU - Vladimirov, M.

AU - Votano, L.

AU - Vuilleumier, J. L.

AU - Wilquet, G.

AU - Wonsak, B.

AU - Yakushev, V.

AU - Yoon, C. S.

AU - Yoshioka, T.

AU - Yoshida, J.

AU - Zaitsev, Y.

AU - Zemskova, S.

AU - Zghiche, A.

AU - Zimmermann, R.

PY - 2010/5/1

Y1 - 2010/5/1

N2 - The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. We computed separately the muon charge ratio for single and for multiple muon events in order to select different energy regions of the primary cosmic ray spectrum and to test the Rμ dependence on the primary composition. The measured Rμ values were corrected taking into account the charge-misidentification errors. Data have also been grouped in five bins of the "vertical surface energy" ℰμcos θ. A fit to a simplified model of muon production in the atmosphere allowed the determination of the pion and kaon charge ratios weighted by the cosmic ray energy spectrum.

AB - The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. We computed separately the muon charge ratio for single and for multiple muon events in order to select different energy regions of the primary cosmic ray spectrum and to test the Rμ dependence on the primary composition. The measured Rμ values were corrected taking into account the charge-misidentification errors. Data have also been grouped in five bins of the "vertical surface energy" ℰμcos θ. A fit to a simplified model of muon production in the atmosphere allowed the determination of the pion and kaon charge ratios weighted by the cosmic ray energy spectrum.

U2 - 10.1140/epjc/s10052-010-1284-8

DO - 10.1140/epjc/s10052-010-1284-8

M3 - Article

AN - SCOPUS:77951766694

SN - 1434-6044

VL - 67

SP - 25

EP - 37

JO - European Physical Journal C

JF - European Physical Journal C

IS - 1

ER -

Measurement of the atmospheric muon charge ratio with the OPERA detector

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