Measurement of the atmospheric muon charge ratio with the OPERA detector

2010-05-01
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.
Brugiere, 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.
Declais, 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, L. S.
Favier, J.
Felici, G.
Ferber, T.
Fini, R.
Frekers, D.
Fukuda, T.
Fukushima, C.
Galkin, V. I.
Garfagnini, A.
Giacomelli, G.
Giorgini, M.
Goellnitz, C.
Goldberg, J.
Golubkov, D.
Goncharova, L.
Gornushkin, Y.
Grella, G.
Grianti, F.
Güler, Ali Murat
Gustavino, C.
Hagner, C.
Hamada, K.
Hara, T.
Hierholzer, M.
Hoshino, K.
Ieva, M.
Jakovcic, K.
Jollet, C.
Juget, F.
Kazuyama, M.
Kim, S. H.
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, M. T.
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, B. D.
Park, I. G.
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.
Parzefall, W. Schmidt
Schroeder, H.
Lavina, L. Scotto
Sheshukov, A.
Shibuya, H.
Simone, S.
Sioli, M.
Sirignano, C.
Sirri, G.
Song, J. S.
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, J. L.
Wilquet, G.
Wonsak, B.
Yakushev, V.
Yoon, C. S.
Yoshioka, T.
Yoshida, J.
Zaitsev, Y.
Zemskova, S.
Zghiche, A.
Zimmermann, R.
The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio R-mu = N-mu+/N-mu- 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-mu dependence on the primary composition. The measured R-mu values were corrected taking into account the charge-misidentification errors. Data have also been grouped in five bins of the "vertical surface energy" epsilon(mu) cos theta. 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.
EUROPEAN PHYSICAL JOURNAL C

Suggestions

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam
Adam, T.; et. al. (2012-10-01)
The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010 and 2011. Dedicated upgrades of the CNGS timing system and of the OPERA detector, as well as a high precision geodesy campaign for the measurement of the neutrino baseline, allowed reaching comparable systematic and statistical accuracies. An arrival time of CNGS muon neu...
Measurement of sm electro-weak parameters in reactor antineutrino-electron scattering in texono experiment
Deniz, Muhammed; Serin, Meltem; Department of Physics (2007)
In this thesis a search for electron type neutrino-electron scattering cross-section and Weinberg Angle measurements were performed at KS Nuclear Power Station with 200 kg CsI(Tl) scintillating crystal detector located at a distance of 28 m from the 2.9 GW reactor core giving total flux of 6:52X10^12 cm^-2s^-1 in average at the experimental site. New analysis techniques and background suppression methods were developed. In the region of 3-8 MeV a measurement of SM cross section of (1:235+-0.577) XR_SM and W...
Measurement of the charge ratio of atmospheric muons with the CMS detector
Khachatryan, V.; et. al. (Elsevier BV, 2010-08-01)
We present a measurement of the ratio of positive to negative muon fluxes from cosmic ray interactions in the atmosphere, using data collected by the CMS detector both at ground level and in the underground experimental cavern at the CERN LHC. Muons were detected in the momentum range from 5 GeV/c to 1 TeV/c. The surface flux ratio is measured to be 1.2766 +/- 0.0032 (stat.) +/- 0.0032 (syst.), independent of the muon momentum, below 100 GeV/c. This is the most precise measurement to date. At higher momenta...
Measurement of v̄e-e- scattering cross-section and constraints on new physics with a CsI(TI) crystal array at the Kuo-Sheng reactor laboratory
Deniz, Muhammed; Bilmiş, Selçuk; Wong, Henry T. (null; 2011-01-01)
The v̄e-e- elastic scattering cross-section was measured with a CsI(Tl) scintillating crystal detector array with a total mass of 187 kg at the Kuo-Sheng Nuclear Power Station. The detectors were exposed to a reactor v̄e flux of 6.4 × 1012 cm-2s-1 originated from a core with 2.9 GW thermal power. The physics motivations, conceptual design, detector hardware, data analysis and background understanding of the experiment are presented. Using 29882/7369 kg-days of Reactor ON/OFF data, the Standard Model (SM) of...
Measurements of D-0 production and of decay branching fractions in neutrino-nucleon scattering
Onengut, G; et. al. (Elsevier BV, 2005-05-05)
During the years 1994-1997, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy. In total about 100 000 charged-current neutrino interactions were located in the nuclear emulsion target and fully reconstructed. From this sample of events which was based on the data acquired by new automatic scanning systems, 1048 charged-current interactions with a Do in the final state were selected by a pattern recognition program and conf...
Citation Formats
N. Agafonova et al., “Measurement of the atmospheric muon charge ratio with the OPERA detector,” EUROPEAN PHYSICAL JOURNAL C, pp. 25–37, 2010, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/69647.