Measurement of the neutrino velocity with the OPERA detector in the CNGS beam
Abstract 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 syst...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adam, T. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Anmerkung: |
© SISSA 2012 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of high energy physics - Berlin : Springer, 1997, 2012(2012), 10 vom: 12. Okt. |
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| Übergeordnetes Werk: |
volume:2012 ; year:2012 ; number:10 ; day:12 ; month:10 |
| Links: |
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| DOI / URN: |
10.1007/JHEP10(2012)093 |
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| Katalog-ID: |
SPR030409284 |
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| 100 | 1 | |a Adam, T. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
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| 520 | |a Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. | ||
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10.1007/JHEP10(2012)093 doi (DE-627)SPR030409284 (SPR)JHEP10(2012)093-e DE-627 ger DE-627 rakwb eng Adam, T. verfasserin aut Measurement of the neutrino velocity with the OPERA detector in the CNGS beam 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA 2012 Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. Neutrino Detectors and Telescopes (dpeaa)DE-He213 Agafonova, N. aut Aleksandrov, A. aut Altinok, O. aut Alvarez Sanchez, P. aut Anokhina, A. aut Aoki, S. aut Ariga, A. aut Ariga, T. aut Autiero, D. aut Badertscher, A. aut Ben Dhahbi, A. aut Bertolin, A. aut Bozza, C. aut Brugière, T. aut Brugnera, R. aut Brunet, F. aut Brunetti, G. aut Buontempo, S. aut Carlus, B. aut Cavanna, F. aut Cazes, A. aut Chaussard, L. aut Chernyavsky, M. aut Chiarella, V. aut Chukanov, A. aut Colosimo, G. aut Crespi, M. aut D’Ambrosio, N. aut De Lellis, G. aut De Serio, M. aut Déclais, Y. aut del Amo Sanchez, P. aut Di Capua, F. aut Di Crescenzo, A. aut Di Ferdinando, D. aut Di Marco, N. aut Dmitrievsky, S. aut Dracos, M. aut Duchesneau, D. aut Dusini, S. aut Dzhatdoev, T. aut Ebert, J. aut Efthymiopoulos, I. aut Egorov, O. aut Ereditato, A. aut Esposito, L. S. aut Favier, J. aut Ferber, T. aut Fini, R. A. aut Fukuda, T. aut Garfagnini, A. aut Giacomelli, G. aut Giorgini, M. aut Giovannozzi, M. aut Girerd, C. aut Goldberg, J. aut Göllnitz, C. aut Golubkov, D. aut Goncharova, L. aut Gornushkin, Y. aut Grella, G. aut Grianti, F. aut Gschwendtner, E. aut Guerin, C. aut Guler, A. M. aut Gustavino, C. aut Hagner, C. aut Hamada, K. aut Hara, T. aut Enikeev, R. aut Hierholzer, M. aut Hollnagel, A. aut Ieva, M. aut Ishida, H. aut Ishiguro, K. aut Jakovcic, K. aut Jollet, C. aut Jones, M. aut Juget, F. aut Kamiscioglu, M. aut Kawada, J. aut Kim, S. H. aut Kimura, M. aut Kiritsis, E. aut Kitagawa, N. aut Klicek, B. aut Knuesel, J. aut Kodama, K. aut Komatsu, M. aut Kose, U. aut Kreslo, I. aut Lazzaro, C. aut Lenkeit, J. aut Ljubicic, A. aut Longhin, A. aut Malgin, A. aut Mandrioli, G. aut Marteau, J. aut Matsuo, T. aut Matveev, V. aut Mauri, N. aut Mazzoni, A. aut Medinaceli, E. aut Meisel, F. aut Meregaglia, A. aut Migliozzi, P. aut Mikado, S. aut Missiaen, D. aut Monacelli, P. aut Morishima, K. aut Moser, U. aut Muciaccia, M. T. aut Naganawa, N. aut Naka, T. aut Nakamura, M. aut Nakano, T. aut Nakatsuka, Y. aut Naumov, D. aut Nikitina, V. aut Nitti, F. aut Ogawa, S. aut Okateva, N. aut Olchevsky, A. aut Palamara, O. aut Paoloni, A. aut Park, B. D. aut Park, I. G. aut Pastore, A. aut Patrizii, L. aut Pennacchio, E. aut Pessard, H. aut Pistillo, C. aut Polukhina, N. aut Pozzato, M. aut Pretzl, K. aut Pupilli, F. aut Rescigno, R. aut Riguzzi, F. aut Roganova, T. aut Rokujo, H. aut Rosa, G. aut Rostovtseva, I. aut Rubbia, A. aut Russo, A. aut Ryasny, V. aut Ryazhskaya, O. aut Sato, O. aut Sato, Y. aut Sahnoun, Z. aut Schembri, A. aut Schuler, J. aut Scotto Lavina, L. aut Serrano, J. aut Shakiryanova, I. aut Sheshukov, A. aut Shibuya, H. aut Shoziyoev, G. aut Simone, S. aut Sioli, M. aut Sirignano, C. aut Sirri, G. aut Song, J. S. aut Spinetti, M. aut Stanco, L. aut Starkov, N. aut Stellacci, S. aut Stipcevic, M. aut Strauss, T. aut Takahashi, S. aut Tenti, M. aut Terranova, F. aut Tezuka, I. aut Tioukov, V. aut Tolun, P. aut Trani, N. T. aut Tufanli, S. aut Vilain, P. aut Vladimirov, M. aut Votano, L. aut Vuilleumier, J.-L. aut Wilquet, G. aut Wonsak, B. aut Wurtz, J. aut Yakushev, V. aut Yoon, C. S. aut Yoshida, J. aut Zaitsev, Y. aut Zemskova, S. aut Zghiche, A. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2012(2012), 10 vom: 12. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2012 year:2012 number:10 day:12 month:10 https://dx.doi.org/10.1007/JHEP10(2012)093 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2012 2012 10 12 10 |
| spelling |
10.1007/JHEP10(2012)093 doi (DE-627)SPR030409284 (SPR)JHEP10(2012)093-e DE-627 ger DE-627 rakwb eng Adam, T. verfasserin aut Measurement of the neutrino velocity with the OPERA detector in the CNGS beam 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA 2012 Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. Neutrino Detectors and Telescopes (dpeaa)DE-He213 Agafonova, N. aut Aleksandrov, A. aut Altinok, O. aut Alvarez Sanchez, P. aut Anokhina, A. aut Aoki, S. aut Ariga, A. aut Ariga, T. aut Autiero, D. aut Badertscher, A. aut Ben Dhahbi, A. aut Bertolin, A. aut Bozza, C. aut Brugière, T. aut Brugnera, R. aut Brunet, F. aut Brunetti, G. aut Buontempo, S. aut Carlus, B. aut Cavanna, F. aut Cazes, A. aut Chaussard, L. aut Chernyavsky, M. aut Chiarella, V. aut Chukanov, A. aut Colosimo, G. aut Crespi, M. aut D’Ambrosio, N. aut De Lellis, G. aut De Serio, M. aut Déclais, Y. aut del Amo Sanchez, P. aut Di Capua, F. aut Di Crescenzo, A. aut Di Ferdinando, D. aut Di Marco, N. aut Dmitrievsky, S. aut Dracos, M. aut Duchesneau, D. aut Dusini, S. aut Dzhatdoev, T. aut Ebert, J. aut Efthymiopoulos, I. aut Egorov, O. aut Ereditato, A. aut Esposito, L. S. aut Favier, J. aut Ferber, T. aut Fini, R. A. aut Fukuda, T. aut Garfagnini, A. aut Giacomelli, G. aut Giorgini, M. aut Giovannozzi, M. aut Girerd, C. aut Goldberg, J. aut Göllnitz, C. aut Golubkov, D. aut Goncharova, L. aut Gornushkin, Y. aut Grella, G. aut Grianti, F. aut Gschwendtner, E. aut Guerin, C. aut Guler, A. M. aut Gustavino, C. aut Hagner, C. aut Hamada, K. aut Hara, T. aut Enikeev, R. aut Hierholzer, M. aut Hollnagel, A. aut Ieva, M. aut Ishida, H. aut Ishiguro, K. aut Jakovcic, K. aut Jollet, C. aut Jones, M. aut Juget, F. aut Kamiscioglu, M. aut Kawada, J. aut Kim, S. H. aut Kimura, M. aut Kiritsis, E. aut Kitagawa, N. aut Klicek, B. aut Knuesel, J. aut Kodama, K. aut Komatsu, M. aut Kose, U. aut Kreslo, I. aut Lazzaro, C. aut Lenkeit, J. aut Ljubicic, A. aut Longhin, A. aut Malgin, A. aut Mandrioli, G. aut Marteau, J. aut Matsuo, T. aut Matveev, V. aut Mauri, N. aut Mazzoni, A. aut Medinaceli, E. aut Meisel, F. aut Meregaglia, A. aut Migliozzi, P. aut Mikado, S. aut Missiaen, D. aut Monacelli, P. aut Morishima, K. aut Moser, U. aut Muciaccia, M. T. aut Naganawa, N. aut Naka, T. aut Nakamura, M. aut Nakano, T. aut Nakatsuka, Y. aut Naumov, D. aut Nikitina, V. aut Nitti, F. aut Ogawa, S. aut Okateva, N. aut Olchevsky, A. aut Palamara, O. aut Paoloni, A. aut Park, B. D. aut Park, I. G. aut Pastore, A. aut Patrizii, L. aut Pennacchio, E. aut Pessard, H. aut Pistillo, C. aut Polukhina, N. aut Pozzato, M. aut Pretzl, K. aut Pupilli, F. aut Rescigno, R. aut Riguzzi, F. aut Roganova, T. aut Rokujo, H. aut Rosa, G. aut Rostovtseva, I. aut Rubbia, A. aut Russo, A. aut Ryasny, V. aut Ryazhskaya, O. aut Sato, O. aut Sato, Y. aut Sahnoun, Z. aut Schembri, A. aut Schuler, J. aut Scotto Lavina, L. aut Serrano, J. aut Shakiryanova, I. aut Sheshukov, A. aut Shibuya, H. aut Shoziyoev, G. aut Simone, S. aut Sioli, M. aut Sirignano, C. aut Sirri, G. aut Song, J. S. aut Spinetti, M. aut Stanco, L. aut Starkov, N. aut Stellacci, S. aut Stipcevic, M. aut Strauss, T. aut Takahashi, S. aut Tenti, M. aut Terranova, F. aut Tezuka, I. aut Tioukov, V. aut Tolun, P. aut Trani, N. T. aut Tufanli, S. aut Vilain, P. aut Vladimirov, M. aut Votano, L. aut Vuilleumier, J.-L. aut Wilquet, G. aut Wonsak, B. aut Wurtz, J. aut Yakushev, V. aut Yoon, C. S. aut Yoshida, J. aut Zaitsev, Y. aut Zemskova, S. aut Zghiche, A. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2012(2012), 10 vom: 12. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2012 year:2012 number:10 day:12 month:10 https://dx.doi.org/10.1007/JHEP10(2012)093 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2012 2012 10 12 10 |
| allfields_unstemmed |
10.1007/JHEP10(2012)093 doi (DE-627)SPR030409284 (SPR)JHEP10(2012)093-e DE-627 ger DE-627 rakwb eng Adam, T. verfasserin aut Measurement of the neutrino velocity with the OPERA detector in the CNGS beam 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA 2012 Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. Neutrino Detectors and Telescopes (dpeaa)DE-He213 Agafonova, N. aut Aleksandrov, A. aut Altinok, O. aut Alvarez Sanchez, P. aut Anokhina, A. aut Aoki, S. aut Ariga, A. aut Ariga, T. aut Autiero, D. aut Badertscher, A. aut Ben Dhahbi, A. aut Bertolin, A. aut Bozza, C. aut Brugière, T. aut Brugnera, R. aut Brunet, F. aut Brunetti, G. aut Buontempo, S. aut Carlus, B. aut Cavanna, F. aut Cazes, A. aut Chaussard, L. aut Chernyavsky, M. aut Chiarella, V. aut Chukanov, A. aut Colosimo, G. aut Crespi, M. aut D’Ambrosio, N. aut De Lellis, G. aut De Serio, M. aut Déclais, Y. aut del Amo Sanchez, P. aut Di Capua, F. aut Di Crescenzo, A. aut Di Ferdinando, D. aut Di Marco, N. aut Dmitrievsky, S. aut Dracos, M. aut Duchesneau, D. aut Dusini, S. aut Dzhatdoev, T. aut Ebert, J. aut Efthymiopoulos, I. aut Egorov, O. aut Ereditato, A. aut Esposito, L. S. aut Favier, J. aut Ferber, T. aut Fini, R. A. aut Fukuda, T. aut Garfagnini, A. aut Giacomelli, G. aut Giorgini, M. aut Giovannozzi, M. aut Girerd, C. aut Goldberg, J. aut Göllnitz, C. aut Golubkov, D. aut Goncharova, L. aut Gornushkin, Y. aut Grella, G. aut Grianti, F. aut Gschwendtner, E. aut Guerin, C. aut Guler, A. M. aut Gustavino, C. aut Hagner, C. aut Hamada, K. aut Hara, T. aut Enikeev, R. aut Hierholzer, M. aut Hollnagel, A. aut Ieva, M. aut Ishida, H. aut Ishiguro, K. aut Jakovcic, K. aut Jollet, C. aut Jones, M. aut Juget, F. aut Kamiscioglu, M. aut Kawada, J. aut Kim, S. H. aut Kimura, M. aut Kiritsis, E. aut Kitagawa, N. aut Klicek, B. aut Knuesel, J. aut Kodama, K. aut Komatsu, M. aut Kose, U. aut Kreslo, I. aut Lazzaro, C. aut Lenkeit, J. aut Ljubicic, A. aut Longhin, A. aut Malgin, A. aut Mandrioli, G. aut Marteau, J. aut Matsuo, T. aut Matveev, V. aut Mauri, N. aut Mazzoni, A. aut Medinaceli, E. aut Meisel, F. aut Meregaglia, A. aut Migliozzi, P. aut Mikado, S. aut Missiaen, D. aut Monacelli, P. aut Morishima, K. aut Moser, U. aut Muciaccia, M. T. aut Naganawa, N. aut Naka, T. aut Nakamura, M. aut Nakano, T. aut Nakatsuka, Y. aut Naumov, D. aut Nikitina, V. aut Nitti, F. aut Ogawa, S. aut Okateva, N. aut Olchevsky, A. aut Palamara, O. aut Paoloni, A. aut Park, B. D. aut Park, I. G. aut Pastore, A. aut Patrizii, L. aut Pennacchio, E. aut Pessard, H. aut Pistillo, C. aut Polukhina, N. aut Pozzato, M. aut Pretzl, K. aut Pupilli, F. aut Rescigno, R. aut Riguzzi, F. aut Roganova, T. aut Rokujo, H. aut Rosa, G. aut Rostovtseva, I. aut Rubbia, A. aut Russo, A. aut Ryasny, V. aut Ryazhskaya, O. aut Sato, O. aut Sato, Y. aut Sahnoun, Z. aut Schembri, A. aut Schuler, J. aut Scotto Lavina, L. aut Serrano, J. aut Shakiryanova, I. aut Sheshukov, A. aut Shibuya, H. aut Shoziyoev, G. aut Simone, S. aut Sioli, M. aut Sirignano, C. aut Sirri, G. aut Song, J. S. aut Spinetti, M. aut Stanco, L. aut Starkov, N. aut Stellacci, S. aut Stipcevic, M. aut Strauss, T. aut Takahashi, S. aut Tenti, M. aut Terranova, F. aut Tezuka, I. aut Tioukov, V. aut Tolun, P. aut Trani, N. T. aut Tufanli, S. aut Vilain, P. aut Vladimirov, M. aut Votano, L. aut Vuilleumier, J.-L. aut Wilquet, G. aut Wonsak, B. aut Wurtz, J. aut Yakushev, V. aut Yoon, C. S. aut Yoshida, J. aut Zaitsev, Y. aut Zemskova, S. aut Zghiche, A. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2012(2012), 10 vom: 12. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2012 year:2012 number:10 day:12 month:10 https://dx.doi.org/10.1007/JHEP10(2012)093 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2012 2012 10 12 10 |
| allfieldsGer |
10.1007/JHEP10(2012)093 doi (DE-627)SPR030409284 (SPR)JHEP10(2012)093-e DE-627 ger DE-627 rakwb eng Adam, T. verfasserin aut Measurement of the neutrino velocity with the OPERA detector in the CNGS beam 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA 2012 Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. Neutrino Detectors and Telescopes (dpeaa)DE-He213 Agafonova, N. aut Aleksandrov, A. aut Altinok, O. aut Alvarez Sanchez, P. aut Anokhina, A. aut Aoki, S. aut Ariga, A. aut Ariga, T. aut Autiero, D. aut Badertscher, A. aut Ben Dhahbi, A. aut Bertolin, A. aut Bozza, C. aut Brugière, T. aut Brugnera, R. aut Brunet, F. aut Brunetti, G. aut Buontempo, S. aut Carlus, B. aut Cavanna, F. aut Cazes, A. aut Chaussard, L. aut Chernyavsky, M. aut Chiarella, V. aut Chukanov, A. aut Colosimo, G. aut Crespi, M. aut D’Ambrosio, N. aut De Lellis, G. aut De Serio, M. aut Déclais, Y. aut del Amo Sanchez, P. aut Di Capua, F. aut Di Crescenzo, A. aut Di Ferdinando, D. aut Di Marco, N. aut Dmitrievsky, S. aut Dracos, M. aut Duchesneau, D. aut Dusini, S. aut Dzhatdoev, T. aut Ebert, J. aut Efthymiopoulos, I. aut Egorov, O. aut Ereditato, A. aut Esposito, L. S. aut Favier, J. aut Ferber, T. aut Fini, R. A. aut Fukuda, T. aut Garfagnini, A. aut Giacomelli, G. aut Giorgini, M. aut Giovannozzi, M. aut Girerd, C. aut Goldberg, J. aut Göllnitz, C. aut Golubkov, D. aut Goncharova, L. aut Gornushkin, Y. aut Grella, G. aut Grianti, F. aut Gschwendtner, E. aut Guerin, C. aut Guler, A. M. aut Gustavino, C. aut Hagner, C. aut Hamada, K. aut Hara, T. aut Enikeev, R. aut Hierholzer, M. aut Hollnagel, A. aut Ieva, M. aut Ishida, H. aut Ishiguro, K. aut Jakovcic, K. aut Jollet, C. aut Jones, M. aut Juget, F. aut Kamiscioglu, M. aut Kawada, J. aut Kim, S. H. aut Kimura, M. aut Kiritsis, E. aut Kitagawa, N. aut Klicek, B. aut Knuesel, J. aut Kodama, K. aut Komatsu, M. aut Kose, U. aut Kreslo, I. aut Lazzaro, C. aut Lenkeit, J. aut Ljubicic, A. aut Longhin, A. aut Malgin, A. aut Mandrioli, G. aut Marteau, J. aut Matsuo, T. aut Matveev, V. aut Mauri, N. aut Mazzoni, A. aut Medinaceli, E. aut Meisel, F. aut Meregaglia, A. aut Migliozzi, P. aut Mikado, S. aut Missiaen, D. aut Monacelli, P. aut Morishima, K. aut Moser, U. aut Muciaccia, M. T. aut Naganawa, N. aut Naka, T. aut Nakamura, M. aut Nakano, T. aut Nakatsuka, Y. aut Naumov, D. aut Nikitina, V. aut Nitti, F. aut Ogawa, S. aut Okateva, N. aut Olchevsky, A. aut Palamara, O. aut Paoloni, A. aut Park, B. D. aut Park, I. G. aut Pastore, A. aut Patrizii, L. aut Pennacchio, E. aut Pessard, H. aut Pistillo, C. aut Polukhina, N. aut Pozzato, M. aut Pretzl, K. aut Pupilli, F. aut Rescigno, R. aut Riguzzi, F. aut Roganova, T. aut Rokujo, H. aut Rosa, G. aut Rostovtseva, I. aut Rubbia, A. aut Russo, A. aut Ryasny, V. aut Ryazhskaya, O. aut Sato, O. aut Sato, Y. aut Sahnoun, Z. aut Schembri, A. aut Schuler, J. aut Scotto Lavina, L. aut Serrano, J. aut Shakiryanova, I. aut Sheshukov, A. aut Shibuya, H. aut Shoziyoev, G. aut Simone, S. aut Sioli, M. aut Sirignano, C. aut Sirri, G. aut Song, J. S. aut Spinetti, M. aut Stanco, L. aut Starkov, N. aut Stellacci, S. aut Stipcevic, M. aut Strauss, T. aut Takahashi, S. aut Tenti, M. aut Terranova, F. aut Tezuka, I. aut Tioukov, V. aut Tolun, P. aut Trani, N. T. aut Tufanli, S. aut Vilain, P. aut Vladimirov, M. aut Votano, L. aut Vuilleumier, J.-L. aut Wilquet, G. aut Wonsak, B. aut Wurtz, J. aut Yakushev, V. aut Yoon, C. S. aut Yoshida, J. aut Zaitsev, Y. aut Zemskova, S. aut Zghiche, A. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2012(2012), 10 vom: 12. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2012 year:2012 number:10 day:12 month:10 https://dx.doi.org/10.1007/JHEP10(2012)093 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2012 2012 10 12 10 |
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10.1007/JHEP10(2012)093 doi (DE-627)SPR030409284 (SPR)JHEP10(2012)093-e DE-627 ger DE-627 rakwb eng Adam, T. verfasserin aut Measurement of the neutrino velocity with the OPERA detector in the CNGS beam 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA 2012 Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. Neutrino Detectors and Telescopes (dpeaa)DE-He213 Agafonova, N. aut Aleksandrov, A. aut Altinok, O. aut Alvarez Sanchez, P. aut Anokhina, A. aut Aoki, S. aut Ariga, A. aut Ariga, T. aut Autiero, D. aut Badertscher, A. aut Ben Dhahbi, A. aut Bertolin, A. aut Bozza, C. aut Brugière, T. aut Brugnera, R. aut Brunet, F. aut Brunetti, G. aut Buontempo, S. aut Carlus, B. aut Cavanna, F. aut Cazes, A. aut Chaussard, L. aut Chernyavsky, M. aut Chiarella, V. aut Chukanov, A. aut Colosimo, G. aut Crespi, M. aut D’Ambrosio, N. aut De Lellis, G. aut De Serio, M. aut Déclais, Y. aut del Amo Sanchez, P. aut Di Capua, F. aut Di Crescenzo, A. aut Di Ferdinando, D. aut Di Marco, N. aut Dmitrievsky, S. aut Dracos, M. aut Duchesneau, D. aut Dusini, S. aut Dzhatdoev, T. aut Ebert, J. aut Efthymiopoulos, I. aut Egorov, O. aut Ereditato, A. aut Esposito, L. S. aut Favier, J. aut Ferber, T. aut Fini, R. A. aut Fukuda, T. aut Garfagnini, A. aut Giacomelli, G. aut Giorgini, M. aut Giovannozzi, M. aut Girerd, C. aut Goldberg, J. aut Göllnitz, C. aut Golubkov, D. aut Goncharova, L. aut Gornushkin, Y. aut Grella, G. aut Grianti, F. aut Gschwendtner, E. aut Guerin, C. aut Guler, A. M. aut Gustavino, C. aut Hagner, C. aut Hamada, K. aut Hara, T. aut Enikeev, R. aut Hierholzer, M. aut Hollnagel, A. aut Ieva, M. aut Ishida, H. aut Ishiguro, K. aut Jakovcic, K. aut Jollet, C. aut Jones, M. aut Juget, F. aut Kamiscioglu, M. aut Kawada, J. aut Kim, S. H. aut Kimura, M. aut Kiritsis, E. aut Kitagawa, N. aut Klicek, B. aut Knuesel, J. aut Kodama, K. aut Komatsu, M. aut Kose, U. aut Kreslo, I. aut Lazzaro, C. aut Lenkeit, J. aut Ljubicic, A. aut Longhin, A. aut Malgin, A. aut Mandrioli, G. aut Marteau, J. aut Matsuo, T. aut Matveev, V. aut Mauri, N. aut Mazzoni, A. aut Medinaceli, E. aut Meisel, F. aut Meregaglia, A. aut Migliozzi, P. aut Mikado, S. aut Missiaen, D. aut Monacelli, P. aut Morishima, K. aut Moser, U. aut Muciaccia, M. T. aut Naganawa, N. aut Naka, T. aut Nakamura, M. aut Nakano, T. aut Nakatsuka, Y. aut Naumov, D. aut Nikitina, V. aut Nitti, F. aut Ogawa, S. aut Okateva, N. aut Olchevsky, A. aut Palamara, O. aut Paoloni, A. aut Park, B. D. aut Park, I. G. aut Pastore, A. aut Patrizii, L. aut Pennacchio, E. aut Pessard, H. aut Pistillo, C. aut Polukhina, N. aut Pozzato, M. aut Pretzl, K. aut Pupilli, F. aut Rescigno, R. aut Riguzzi, F. aut Roganova, T. aut Rokujo, H. aut Rosa, G. aut Rostovtseva, I. aut Rubbia, A. aut Russo, A. aut Ryasny, V. aut Ryazhskaya, O. aut Sato, O. aut Sato, Y. aut Sahnoun, Z. aut Schembri, A. aut Schuler, J. aut Scotto Lavina, L. aut Serrano, J. aut Shakiryanova, I. aut Sheshukov, A. aut Shibuya, H. aut Shoziyoev, G. aut Simone, S. aut Sioli, M. aut Sirignano, C. aut Sirri, G. aut Song, J. S. aut Spinetti, M. aut Stanco, L. aut Starkov, N. aut Stellacci, S. aut Stipcevic, M. aut Strauss, T. aut Takahashi, S. aut Tenti, M. aut Terranova, F. aut Tezuka, I. aut Tioukov, V. aut Tolun, P. aut Trani, N. T. aut Tufanli, S. aut Vilain, P. aut Vladimirov, M. aut Votano, L. aut Vuilleumier, J.-L. aut Wilquet, G. aut Wonsak, B. aut Wurtz, J. aut Yakushev, V. aut Yoon, C. S. aut Yoshida, J. aut Zaitsev, Y. aut Zemskova, S. aut Zghiche, A. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2012(2012), 10 vom: 12. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2012 year:2012 number:10 day:12 month:10 https://dx.doi.org/10.1007/JHEP10(2012)093 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2012 2012 10 12 10 |
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Adam, T. @@aut@@ Agafonova, N. @@aut@@ Aleksandrov, A. @@aut@@ Altinok, O. @@aut@@ Alvarez Sanchez, P. @@aut@@ Anokhina, A. @@aut@@ Aoki, S. @@aut@@ Ariga, A. @@aut@@ Ariga, T. @@aut@@ Autiero, D. @@aut@@ Badertscher, A. @@aut@@ Ben Dhahbi, A. @@aut@@ Bertolin, A. @@aut@@ Bozza, C. @@aut@@ Brugière, T. @@aut@@ Brugnera, R. @@aut@@ Brunet, F. @@aut@@ Brunetti, G. @@aut@@ Buontempo, S. @@aut@@ Carlus, B. @@aut@@ Cavanna, F. @@aut@@ Cazes, A. @@aut@@ Chaussard, L. @@aut@@ Chernyavsky, M. @@aut@@ Chiarella, V. @@aut@@ Chukanov, A. @@aut@@ Colosimo, G. @@aut@@ Crespi, M. @@aut@@ D’Ambrosio, N. @@aut@@ De Lellis, G. @@aut@@ De Serio, M. @@aut@@ Déclais, Y. @@aut@@ del Amo Sanchez, P. @@aut@@ Di Capua, F. @@aut@@ Di Crescenzo, A. @@aut@@ Di Ferdinando, D. @@aut@@ Di Marco, N. @@aut@@ Dmitrievsky, S. @@aut@@ Dracos, M. @@aut@@ Duchesneau, D. @@aut@@ Dusini, S. @@aut@@ Dzhatdoev, T. @@aut@@ Ebert, J. @@aut@@ Efthymiopoulos, I. @@aut@@ Egorov, O. @@aut@@ Ereditato, A. @@aut@@ Esposito, L. S. @@aut@@ Favier, J. @@aut@@ Ferber, T. @@aut@@ Fini, R. A. @@aut@@ Fukuda, T. @@aut@@ Garfagnini, A. @@aut@@ Giacomelli, G. @@aut@@ Giorgini, M. @@aut@@ Giovannozzi, M. @@aut@@ Girerd, C. @@aut@@ Goldberg, J. @@aut@@ Göllnitz, C. @@aut@@ Golubkov, D. @@aut@@ Goncharova, L. @@aut@@ Gornushkin, Y. @@aut@@ Grella, G. @@aut@@ Grianti, F. @@aut@@ Gschwendtner, E. @@aut@@ Guerin, C. @@aut@@ Guler, A. M. @@aut@@ Gustavino, C. @@aut@@ Hagner, C. @@aut@@ Hamada, K. @@aut@@ Hara, T. @@aut@@ Enikeev, R. @@aut@@ Hierholzer, M. @@aut@@ Hollnagel, A. @@aut@@ Ieva, M. @@aut@@ Ishida, H. @@aut@@ Ishiguro, K. @@aut@@ Jakovcic, K. @@aut@@ Jollet, C. @@aut@@ Jones, M. @@aut@@ Juget, F. @@aut@@ Kamiscioglu, M. @@aut@@ Kawada, J. @@aut@@ Kim, S. H. @@aut@@ Kimura, M. @@aut@@ Kiritsis, E. @@aut@@ Kitagawa, N. @@aut@@ Klicek, B. @@aut@@ Knuesel, J. @@aut@@ Kodama, K. @@aut@@ Komatsu, M. @@aut@@ Kose, U. @@aut@@ Kreslo, I. @@aut@@ Lazzaro, C. @@aut@@ Lenkeit, J. @@aut@@ Ljubicic, A. @@aut@@ Longhin, A. @@aut@@ Malgin, A. @@aut@@ Mandrioli, G. @@aut@@ Marteau, J. @@aut@@ Matsuo, T. @@aut@@ Matveev, V. @@aut@@ Mauri, N. @@aut@@ Mazzoni, A. @@aut@@ Medinaceli, E. @@aut@@ Meisel, F. @@aut@@ Meregaglia, A. @@aut@@ Migliozzi, P. @@aut@@ Mikado, S. @@aut@@ Missiaen, D. @@aut@@ Monacelli, P. @@aut@@ Morishima, K. @@aut@@ Moser, U. @@aut@@ Muciaccia, M. T. @@aut@@ Naganawa, N. @@aut@@ Naka, T. @@aut@@ Nakamura, M. @@aut@@ Nakano, T. @@aut@@ Nakatsuka, Y. @@aut@@ Naumov, D. @@aut@@ Nikitina, V. @@aut@@ Nitti, F. @@aut@@ Ogawa, S. @@aut@@ Okateva, N. @@aut@@ Olchevsky, A. @@aut@@ Palamara, O. @@aut@@ Paoloni, A. @@aut@@ Park, B. D. @@aut@@ Park, I. G. @@aut@@ Pastore, A. @@aut@@ Patrizii, L. @@aut@@ Pennacchio, E. @@aut@@ Pessard, H. @@aut@@ Pistillo, C. @@aut@@ Polukhina, N. @@aut@@ Pozzato, M. @@aut@@ Pretzl, K. @@aut@@ Pupilli, F. @@aut@@ Rescigno, R. @@aut@@ Riguzzi, F. @@aut@@ Roganova, T. @@aut@@ Rokujo, H. @@aut@@ Rosa, G. @@aut@@ Rostovtseva, I. @@aut@@ Rubbia, A. @@aut@@ Russo, A. @@aut@@ Ryasny, V. @@aut@@ Ryazhskaya, O. @@aut@@ Sato, O. @@aut@@ Sato, Y. @@aut@@ Sahnoun, Z. @@aut@@ Schembri, A. @@aut@@ Schuler, J. @@aut@@ Scotto Lavina, L. @@aut@@ Serrano, J. @@aut@@ Shakiryanova, I. @@aut@@ Sheshukov, A. @@aut@@ Shibuya, H. @@aut@@ Shoziyoev, G. @@aut@@ Simone, S. @@aut@@ Sioli, M. @@aut@@ Sirignano, C. @@aut@@ Sirri, G. @@aut@@ Song, J. S. @@aut@@ Spinetti, M. @@aut@@ Stanco, L. @@aut@@ Starkov, N. @@aut@@ Stellacci, S. @@aut@@ Stipcevic, M. @@aut@@ Strauss, T. @@aut@@ Takahashi, S. @@aut@@ Tenti, M. @@aut@@ Terranova, F. @@aut@@ Tezuka, I. @@aut@@ Tioukov, V. @@aut@@ Tolun, P. @@aut@@ Trani, N. T. @@aut@@ Tufanli, S. @@aut@@ Vilain, P. @@aut@@ Vladimirov, M. @@aut@@ Votano, L. @@aut@@ Vuilleumier, J.-L. @@aut@@ Wilquet, G. @@aut@@ Wonsak, B. @@aut@@ Wurtz, J. @@aut@@ Yakushev, V. @@aut@@ Yoon, C. S. @@aut@@ Yoshida, J. @@aut@@ Zaitsev, Y. @@aut@@ Zemskova, S. @@aut@@ Zghiche, A. @@aut@@ |
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Adam, T. |
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Adam, T. misc Neutrino Detectors and Telescopes Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
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Measurement of the neutrino velocity with the OPERA detector in the CNGS beam Neutrino Detectors and Telescopes (dpeaa)DE-He213 |
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Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
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Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
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Adam, T. Agafonova, N. Aleksandrov, A. Altinok, O. Alvarez Sanchez, P. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Autiero, D. Badertscher, A. Ben Dhahbi, A. Bertolin, A. Bozza, C. Brugière, T. Brugnera, R. Brunet, F. Brunetti, G. Buontempo, S. Carlus, B. Cavanna, F. Cazes, A. Chaussard, L. Chernyavsky, M. Chiarella, V. Chukanov, A. Colosimo, G. Crespi, M. D’Ambrosio, N. De Lellis, G. De Serio, M. Déclais, Y. del Amo Sanchez, P. Di Capua, F. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Efthymiopoulos, I. Egorov, O. Ereditato, A. Esposito, L. S. Favier, J. Ferber, T. Fini, R. A. Fukuda, T. Garfagnini, A. Giacomelli, G. Giorgini, M. Giovannozzi, M. Girerd, C. Goldberg, J. Göllnitz, C. Golubkov, D. Goncharova, L. Gornushkin, Y. Grella, G. Grianti, F. Gschwendtner, E. Guerin, C. Guler, A. M. Gustavino, C. Hagner, C. Hamada, K. Hara, T. Enikeev, R. Hierholzer, M. Hollnagel, A. Ieva, M. Ishida, H. Ishiguro, K. Jakovcic, K. Jollet, C. Jones, M. Juget, F. Kamiscioglu, M. Kawada, J. Kim, S. H. Kimura, M. Kiritsis, E. Kitagawa, N. Klicek, B. Knuesel, J. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Lazzaro, C. Lenkeit, J. Ljubicic, A. Longhin, A. Malgin, A. Mandrioli, G. Marteau, J. Matsuo, T. Matveev, V. Mauri, N. Mazzoni, A. Medinaceli, E. Meisel, F. Meregaglia, A. Migliozzi, P. Mikado, S. Missiaen, D. Monacelli, P. Morishima, K. Moser, U. Muciaccia, M. T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Nakatsuka, Y. Naumov, D. Nikitina, V. Nitti, F. Ogawa, S. Okateva, N. Olchevsky, A. Palamara, O. Paoloni, A. Park, B. D. Park, I. G. Pastore, A. Patrizii, L. Pennacchio, E. Pessard, H. Pistillo, C. Polukhina, N. Pozzato, M. Pretzl, K. Pupilli, F. Rescigno, R. Riguzzi, F. Roganova, T. Rokujo, H. Rosa, G. Rostovtseva, I. Rubbia, A. Russo, A. Ryasny, V. Ryazhskaya, O. Sato, O. Sato, Y. Sahnoun, Z. Schembri, A. Schuler, J. Scotto Lavina, L. Serrano, J. Shakiryanova, I. Sheshukov, A. Shibuya, H. Shoziyoev, G. Simone, S. Sioli, M. Sirignano, C. Sirri, G. Song, J. S. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S. Stipcevic, M. Strauss, T. Takahashi, S. Tenti, M. Terranova, F. Tezuka, I. Tioukov, V. Tolun, P. Trani, N. T. Tufanli, S. Vilain, P. Vladimirov, M. Votano, L. Vuilleumier, J.-L. Wilquet, G. Wonsak, B. Wurtz, J. Yakushev, V. Yoon, C. S. Yoshida, J. Zaitsev, Y. Zemskova, S. Zghiche, A. |
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Elektronische Aufsätze |
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Adam, T. |
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10.1007/JHEP10(2012)093 |
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measurement of the neutrino velocity with the opera detector in the cngs beam |
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Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
| abstract |
Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. © SISSA 2012 |
| abstractGer |
Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. © SISSA 2012 |
| abstract_unstemmed |
Abstract 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 neutrinos with respect to the one computed assuming the speed of light in vacuum of $ \left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns} $ was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light $ {{{\left( {\silon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }} $. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level. © SISSA 2012 |
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| title_short |
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam |
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https://dx.doi.org/10.1007/JHEP10(2012)093 |
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Agafonova, N. Aleksandrov, A. Altinok, O. Alvarez Sanchez, P. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Autiero, D. Badertscher, A. Ben Dhahbi, A. Bertolin, A. Bozza, C. Brugière, T. Brugnera, R. Brunet, F. Brunetti, G. Buontempo, S. Carlus, B. Cavanna, F. Cazes, A. Chaussard, L. Chernyavsky, M. Chiarella, V. Chukanov, A. Colosimo, G. Crespi, M. D’Ambrosio, N. De Lellis, G. De Serio, M. Déclais, Y. del Amo Sanchez, P. Di Capua, F. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Efthymiopoulos, I. Egorov, O. Ereditato, A. Esposito, L. S. Favier, J. Ferber, T. Fini, R. A. Fukuda, T. Garfagnini, A. Giacomelli, G. Giorgini, M. Giovannozzi, M. Girerd, C. Goldberg, J. Göllnitz, C. Golubkov, D. Goncharova, L. Gornushkin, Y. Grella, G. Grianti, F. Gschwendtner, E. Guerin, C. Guler, A. M. Gustavino, C. Hagner, C. Hamada, K. Hara, T. Enikeev, R. Hierholzer, M. Hollnagel, A. Ieva, M. Ishida, H. Ishiguro, K. Jakovcic, K. Jollet, C. Jones, M. Juget, F. Kamiscioglu, M. Kawada, J. Kim, S. H. Kimura, M. Kiritsis, E. Kitagawa, N. Klicek, B. Knuesel, J. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Lazzaro, C. Lenkeit, J. Ljubicic, A. Longhin, A. Malgin, A. Mandrioli, G. Marteau, J. Matsuo, T. Matveev, V. Mauri, N. Mazzoni, A. Medinaceli, E. Meisel, F. Meregaglia, A. Migliozzi, P. Mikado, S. Missiaen, D. Monacelli, P. Morishima, K. Moser, U. Muciaccia, M. T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Nakatsuka, Y. Naumov, D. Nikitina, V. Nitti, F. Ogawa, S. Okateva, N. Olchevsky, A. Palamara, O. Paoloni, A. Park, B. D. Park, I. G. Pastore, A. Patrizii, L. Pennacchio, E. Pessard, H. Pistillo, C. Polukhina, N. Pozzato, M. Pretzl, K. Pupilli, F. Rescigno, R. Riguzzi, F. Roganova, T. Rokujo, H. Rosa, G. Rostovtseva, I. Rubbia, A. Russo, A. Ryasny, V. Ryazhskaya, O. Sato, O. Sato, Y. Sahnoun, Z. Schembri, A. Schuler, J. Scotto Lavina, L. Serrano, J. Shakiryanova, I. Sheshukov, A. Shibuya, H. Shoziyoev, G. Simone, S. Sioli, M. Sirignano, C. Sirri, G. Song, J. S. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S. Stipcevic, M. Strauss, T. Takahashi, S. Tenti, M. Terranova, F. Tezuka, I. Tioukov, V. Tolun, P. Trani, N. T. Tufanli, S. Vilain, P. Vladimirov, M. Votano, L. Vuilleumier, J.-L. Wilquet, G. Wonsak, B. Wurtz, J. Yakushev, V. Yoon, C. S. Yoshida, J. Zaitsev, Y. Zemskova, S. Zghiche, A. |
| author2Str |
Agafonova, N. Aleksandrov, A. Altinok, O. Alvarez Sanchez, P. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Autiero, D. Badertscher, A. Ben Dhahbi, A. Bertolin, A. Bozza, C. Brugière, T. Brugnera, R. Brunet, F. Brunetti, G. Buontempo, S. Carlus, B. Cavanna, F. Cazes, A. Chaussard, L. Chernyavsky, M. Chiarella, V. Chukanov, A. Colosimo, G. Crespi, M. D’Ambrosio, N. De Lellis, G. De Serio, M. Déclais, Y. del Amo Sanchez, P. Di Capua, F. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Efthymiopoulos, I. Egorov, O. Ereditato, A. Esposito, L. S. Favier, J. Ferber, T. Fini, R. A. Fukuda, T. Garfagnini, A. Giacomelli, G. Giorgini, M. Giovannozzi, M. Girerd, C. Goldberg, J. Göllnitz, C. Golubkov, D. Goncharova, L. Gornushkin, Y. Grella, G. Grianti, F. Gschwendtner, E. Guerin, C. Guler, A. M. Gustavino, C. Hagner, C. Hamada, K. Hara, T. Enikeev, R. Hierholzer, M. Hollnagel, A. Ieva, M. Ishida, H. Ishiguro, K. Jakovcic, K. Jollet, C. Jones, M. Juget, F. Kamiscioglu, M. Kawada, J. Kim, S. H. Kimura, M. Kiritsis, E. Kitagawa, N. Klicek, B. Knuesel, J. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Lazzaro, C. Lenkeit, J. Ljubicic, A. Longhin, A. Malgin, A. Mandrioli, G. Marteau, J. Matsuo, T. Matveev, V. Mauri, N. Mazzoni, A. Medinaceli, E. Meisel, F. Meregaglia, A. Migliozzi, P. Mikado, S. Missiaen, D. Monacelli, P. Morishima, K. Moser, U. Muciaccia, M. T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Nakatsuka, Y. Naumov, D. Nikitina, V. Nitti, F. Ogawa, S. Okateva, N. Olchevsky, A. Palamara, O. Paoloni, A. Park, B. D. Park, I. G. Pastore, A. Patrizii, L. Pennacchio, E. Pessard, H. Pistillo, C. Polukhina, N. Pozzato, M. Pretzl, K. Pupilli, F. Rescigno, R. Riguzzi, F. Roganova, T. Rokujo, H. Rosa, G. Rostovtseva, I. Rubbia, A. Russo, A. Ryasny, V. Ryazhskaya, O. Sato, O. Sato, Y. Sahnoun, Z. Schembri, A. Schuler, J. Scotto Lavina, L. Serrano, J. Shakiryanova, I. Sheshukov, A. Shibuya, H. Shoziyoev, G. Simone, S. Sioli, M. Sirignano, C. Sirri, G. Song, J. S. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S. Stipcevic, M. Strauss, T. Takahashi, S. Tenti, M. Terranova, F. Tezuka, I. Tioukov, V. Tolun, P. Trani, N. T. Tufanli, S. Vilain, P. Vladimirov, M. Votano, L. Vuilleumier, J.-L. Wilquet, G. Wonsak, B. Wurtz, J. Yakushev, V. Yoon, C. S. Yoshida, J. Zaitsev, Y. Zemskova, S. Zghiche, A. |
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| score |
7.3998547 |