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Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam
OPERA is a long-baseline experiment designed to search for$\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at theINFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGSneutrino beam from CERN. After the discovery of $\nu_\tau$ appearance in 2015,with $5....
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Lenguaje: | eng |
Publicado: |
2018
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.21468/SciPostPhysProc.1.028 http://cds.cern.ch/record/2645902 |
_version_ | 1780960457067069440 |
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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. Gorbunov, S. Gornushkin, Y. 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. Longhin, A. Loverre, P. Malenica, M. Malgin, A. 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. Ogawa, S. Olchevsky, A. Okateva, N. 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. Shibayama, E. Shibuya, H. 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. Gorbunov, S. Gornushkin, Y. 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. Longhin, A. Loverre, P. Malenica, M. Malgin, A. 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. Ogawa, S. Olchevsky, A. Okateva, N. 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. Shibayama, E. Shibuya, H. 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 | OPERA is a long-baseline experiment designed to search for$\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at theINFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGSneutrino beam from CERN. After the discovery of $\nu_\tau$ appearance in 2015,with $5.1\sigma$ significance, the criteria to select $\nu_\tau$ candidateshave been extended and a multivariate approach has been used for eventsidentification. In this way the statistical uncertainty in the measurement ofthe oscillation parameters and of $\nu_\tau$ properties has been improved.Results are reported. |
id | cern-2645902 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2018 |
record_format | invenio |
spelling | cern-26459022023-04-04T03:12:39Zdoi:10.21468/SciPostPhysProc.1.028http://cds.cern.ch/record/2645902engAgafonova, 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.Gorbunov, S.Gornushkin, Y.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.Longhin, A.Loverre, P.Malenica, M.Malgin, A.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.Ogawa, S.Olchevsky, A.Okateva, N.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.Shibayama, E.Shibuya, H.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.Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beamphysics.ins-detDetectors and Experimental Techniqueshep-exParticle Physics - ExperimentOPERA is a long-baseline experiment designed to search for$\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at theINFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGSneutrino beam from CERN. After the discovery of $\nu_\tau$ appearance in 2015,with $5.1\sigma$ significance, the criteria to select $\nu_\tau$ candidateshave been extended and a multivariate approach has been used for eventsidentification. In this way the statistical uncertainty in the measurement ofthe oscillation parameters and of $\nu_\tau$ properties has been improved.Results are reported.OPERA is a long-baseline experiment designed to search for $\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at the INFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGS neutrino beam from CERN. After the discovery of $\nu_\tau$ appearance in 2015, with $5.1\sigma$ significance, the criteria to select $\nu_\tau$ candidates have been extended and a multivariate approach has been used for events identification. In this way the statistical uncertainty in the measurement of the oscillation parameters and of $\nu_\tau$ properties has been improved. Results are reported.arXiv:1811.00095oai:cds.cern.ch:26459022018-10-31 |
spellingShingle | physics.ins-det Detectors and Experimental Techniques 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. Gorbunov, S. Gornushkin, Y. 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. Longhin, A. Loverre, P. Malenica, M. Malgin, A. 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. Ogawa, S. Olchevsky, A. Okateva, N. 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. Shibayama, E. Shibuya, H. 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. Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title | Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title_full | Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title_fullStr | Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title_full_unstemmed | Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title_short | Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam |
title_sort | latest results of the opera experiment on nu-tau appearance in the cngs neutrino beam |
topic | physics.ins-det Detectors and Experimental Techniques hep-ex Particle Physics - Experiment |
url | https://dx.doi.org/10.21468/SciPostPhysProc.1.028 http://cds.cern.ch/record/2645902 |
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