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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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Detalles Bibliográficos
Autores principales: 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.
Lenguaje:eng
Publicado: 2018
Materias:
Acceso en línea:https://dx.doi.org/10.21468/SciPostPhysProc.1.028
http://cds.cern.ch/record/2645902
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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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AT miyanishim latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT mizutanif latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT monacellip latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT montesimc latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT morishimak latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT muciacciamt latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT naganawan latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT nakat latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT nakamuram latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT nakanot latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT niwak latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT ogawas latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT olchevskya latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT okatevan latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT ozakik latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT paolonia latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT paparellal latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT parkbd latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pasqualinil latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pastorea latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT patriziil latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pessardh latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pistilloc latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT podgrudkovd latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT polukhinan latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pozzatom latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT pupillif latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT rodam latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT roganovat latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT rokujoh latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT rosag latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT ryazhskayao latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT sadovskya latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT satoo latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT schembria latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT shakiryanovai latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT shchedrinat latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT shibayamae latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT shibuyah latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT shiraishit latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT simones latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT sirignanoc latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT sirrig latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT sotnikova latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT spinettim latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT stancol latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT starkovn latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT stellaccism latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT stipcevicm latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT strolinp latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT takahashis latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT tentim latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT terranovaf latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT tioukovv latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT tufanlis latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT ustyuzhanina latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT vasinas latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT vilainp latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT voevodinae latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT votanol latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT vuilleumierjl latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT wilquetg latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT wonsakb latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam
AT yooncs latestresultsoftheoperaexperimentonnutauappearanceinthecngsneutrinobeam