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Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam
The OPERA experiment was designed to study νμ→ντ oscillations in the appearance mode in the CERN to Gran Sasso Neutrino beam (CNGS). In this Letter, we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to 17.97×1019 protons on target. Selection criteria...
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| Lenguaje: | eng |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.120.211801 https://dx.doi.org/10.1103/PhysRevLett.121.139901 http://cds.cern.ch/record/2313639 |
| _version_ | 1780958054054887424 |
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| author | 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. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Favier, J. Fini, R.A. Fornari, F. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gornushkin, Y. Gorbunov, S. 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. Malenica, M. 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. Okateva, N. Olchevsky, A. Ogawa, S. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Pistillo, C. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Roda, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sadovsky, A. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibuya, H. Shibayama, E. 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. Tufanli, S. Ustyuzhanin, A. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Wonsak, B. Yoon, C.S. |
| author_facet | 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. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Favier, J. Fini, R.A. Fornari, F. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gornushkin, Y. Gorbunov, S. 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. Malenica, M. 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. Okateva, N. Olchevsky, A. Ogawa, S. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Pistillo, C. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Roda, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sadovsky, A. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibuya, H. Shibayama, E. 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. Tufanli, S. Ustyuzhanin, A. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Wonsak, B. Yoon, C.S. |
| author_sort | Agafonova, N. |
| collection | CERN |
| description | The OPERA experiment was designed to study νμ→ντ oscillations in the appearance mode in the CERN to Gran Sasso Neutrino beam (CNGS). In this Letter, we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to 17.97×1019 protons on target. Selection criteria looser than in previous analyses have produced ten ντ candidate events, thus reducing the statistical uncertainty in the measurement of the oscillation parameters and of ντ properties. A multivariate approach for event identification has been applied to the candidate events and the discovery of ντ appearance is confirmed with an improved significance level of 6.1σ. |Δm322| has been measured, in appearance mode, with an accuracy of 20%. The measurement of the ντ charged-current cross section, for the first time with a negligible contamination from ν¯τ, and the first direct evidence for the ντ lepton number are also reported. |
| id | cern-2313639 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2018 |
| record_format | invenio |
| spelling | cern-23136392023-04-04T03:36:02Zdoi:10.1103/PhysRevLett.120.211801doi:10.1103/PhysRevLett.121.139901http://cds.cern.ch/record/2313639engAgafonova, 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.De Lellis, G.De Serio, M.del Amo Sanchez, P.Di Crescenzo, A.Di Ferdinando, D.Di Marco, N.Dmitrievsky, S.Dracos, M.Duchesneau, D.Dusini, S.Dzhatdoev, T.Ebert, J.Ereditato, A.Favier, J.Fini, R.A.Fornari, F.Fukuda, T.Galati, G.Garfagnini, A.Gentile, V.Goldberg, J.Gornushkin, Y.Gorbunov, S.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.Malenica, M.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.Okateva, N.Olchevsky, A.Ogawa, S.Ozaki, K.Paoloni, A.Paparella, L.Park, B.D.Pasqualini, L.Pastore, A.Patrizii, L.Pessard, H.Pistillo, C.Podgrudkov, D.Polukhina, N.Pozzato, M.Pupilli, F.Roda, M.Roganova, T.Rokujo, H.Rosa, G.Ryazhskaya, O.Sadovsky, A.Sato, O.Schembri, A.Shakiryanova, I.Shchedrina, T.Shibuya, H.Shibayama, E.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.Tufanli, S.Ustyuzhanin, A.Vasina, S.Vilain, P.Voevodina, E.Votano, L.Vuilleumier, J.L.Wilquet, G.Wonsak, B.Yoon, C.S.Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beamhep-exParticle Physics - ExperimentThe OPERA experiment was designed to study νμ→ντ oscillations in the appearance mode in the CERN to Gran Sasso Neutrino beam (CNGS). In this Letter, we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to 17.97×1019 protons on target. Selection criteria looser than in previous analyses have produced ten ντ candidate events, thus reducing the statistical uncertainty in the measurement of the oscillation parameters and of ντ properties. A multivariate approach for event identification has been applied to the candidate events and the discovery of ντ appearance is confirmed with an improved significance level of 6.1σ. |Δm322| has been measured, in appearance mode, with an accuracy of 20%. The measurement of the ντ charged-current cross section, for the first time with a negligible contamination from ν¯τ, and the first direct evidence for the ντ lepton number are also reported.The OPERA experiment was designed to study $\nu_\mu\to\nu_\tau$ oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to $17.97\cdot 10^{19}$ protons on target. Selection criteria looser than in previous analyses have produced ten $\nu_\tau$ candidate events, thus reducing the statistical uncertainty in the measurement of the oscillation parameters and of $\nu_\tau$ properties. A multivariate approach for event identification has been applied to the candidate events and the discovery of $\nu_\tau$ appearance is confirmed with an improved significance level of 6.1 $\sigma$. $\Delta m^2_{23}$ has been measured, in appearance mode, with an accuracy of 20%. The measurement of $\nu_\tau$ CC cross-section, for the first time with a negligible contamination from $\bar{\nu}_\tau$, and the first direct observation of the $\nu_\tau$ lepton number are also reported.arXiv:1804.04912oai:cds.cern.ch:23136392018-04-13 |
| spellingShingle | hep-ex Particle Physics - Experiment 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. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Favier, J. Fini, R.A. Fornari, F. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gornushkin, Y. Gorbunov, S. 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. Malenica, M. 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. Okateva, N. Olchevsky, A. Ogawa, S. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Pistillo, C. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Roda, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sadovsky, A. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibuya, H. Shibayama, E. 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. Tufanli, S. Ustyuzhanin, A. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Wonsak, B. Yoon, C.S. Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title | Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title_full | Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title_fullStr | Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title_full_unstemmed | Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title_short | Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam |
| title_sort | final results of the opera experiment on $\nu_\tau$ appearance in the cngs beam |
| topic | hep-ex Particle Physics - Experiment |
| url | https://dx.doi.org/10.1103/PhysRevLett.120.211801 https://dx.doi.org/10.1103/PhysRevLett.121.139901 http://cds.cern.ch/record/2313639 |
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