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Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam

Authors :
Mitsuhiro Nakamura
R. Brugnera
Toshiyuki Nakano
Cristiano Bozza
M. Tenti
N. M. Okateva
Kimio Niwa
F. Pupilli
V. Gentile
Tomoko Ariga
M. De Serio
Antonio Ereditato
Kunihiro Morishima
G. De Lellis
N. Di Marco
I. Shakiryanova
Timur Dzhatdoev
A. Sotnikov
Masahiro Komatsu
Krešimir Jakovčić
Nicola D'Ambrosio
Caren Hagner
T. Naka
A. Hollnagel
L. Paparella
M. Spinetti
D. A. Podgrudkov
Gaston Wilquet
A. Di Crescenzo
A. Garfagnini
H. Shibuya
L. Consiglio
L. Pasqualini
F. Terranova
G. Sirri
E. Shibayama
P. Monacelli
B. Klicek
Akitaka Ariga
S. Simone
C. Gustavino
Artem Chukanov
T. Fukuda
N. I. Starkov
D. Duchesneau
Utku Kose
E. Voevodina
M. Chernyavskiy
T. M. Roganova
Alessandro Paoloni
F. Mizutani
L. Patrizii
Natalia Polukhina
C. Kamiscioglu
N. Agafonova
J. L. Vuilleumier
J. Goldberg
Osamu Sato
N. Mauri
Shigeki Aoki
Adele Lauria
S. Dmitrievsky
B. D. Park
G. Mandrioli
T. Shiraishi
A. Iuliano
O. G. Ryazhskaya
H. Pessard
Luca Stanco
V. Matveev
G. Grella
A. Longhin
Valeri Tioukov
Pierre Vilain
K. Kodama
E. Medinaceli
S. Dusini
G. Galati
J. Ebert
P. del Amo Sanchez
Hiroki Rokujo
A. Schembri
Y. A. Gornushkin
C. S. Yoon
Salvatore Buontempo
Simona Maria Stellacci
L. Votano
S. Vasina
Kazumi Ozaki
Maria Cristina Montesi
Chiara Sirignano
P. F. Loverre
A. S. Malgin
Satoru Takahashi
Gianfranca De Rosa
Naotaka Naganawa
T. Hayakawa
Anselmo Meregaglia
F. Laudisio
Seok Kim
M. Roda
M. Pozzato
S. Gorbunov
P. Strolin
M. Kamiscioglu
Marcos Dracos
A. M. Anokhina
T. V. Shchedrina
S. Ogawa
S. Tufanli
Cécile Jollet
A. Alexandrov
M. T. Muciaccia
A. M. Guler
I. Kreslo
Alessandro Pastore
Mario Stipčević
Katsumi Ishiguro
Motoaki Miyanishi
R. A. Fini
Nobuko Kitagawa
T. Matsuo
A. Bertolin
T. Hara
D. Di Ferdinando
S. Mikado
Agafonova, N.
Alexandrov, A.
Anokhina, A.
Aoki, S.
Ariga, A.
Ariga, T.
Bertolin, A.
Bozza, C.
Brugnera, R.
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.
Fini, R. A.
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.
Jakovčić, K.
Jollet, C.
Kamiscioglu, C.
Kamiscioglu, M.
Kim, S. H.
Kitagawa, N.
Kliček, B.
Kodama, K.
Komatsu, M.
Kose, U.
Kreslo, I.
Laudisio, F.
Lauria, A.
Longhin, A.
Loverre, P.
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.
Okateva, N.
Ozaki, K.
Paoloni, A.
Paparella, L.
Park, B. D.
Pasqualini, L.
Pastore, A.
Patrizii, L.
Pessard, H.
Podgrudkov, D.
Polukhina, N.
Pozzato, M.
Pupilli, F.
Roda, M.
Roganova, T.
Rokujo, H.
Rosa, G.
Ryazhskaya, O.
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.
Stipčević, M.
Strolin, P.
Takahashi, S.
Tenti, M.
Terranova, F.
Tioukov, V.
Tufanli, S.
Vasina, S.
Vilain, P.
Voevodina, E.
Votano, L.
Vuilleumier, J. L.
Wilquet, G.
Yoon, C. S.
Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)
Institut Pluridisciplinaire Hubert Curien (IPHC)
Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)
OPERA
Agafonova, N
Alexandrov, A
Anokhina, A
Aoki, S
Ariga, A
Ariga, T
Bertolin, A
Bozza, C
Brugnera, R
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
Fini, R
Fukuda, T
Galati, G
Garfagnini, A
Gentile, V
Goldberg, J
Gorbunov, S
Gornushkin, Y
Grella, G
Guler, A
Gustavino, C
Hagner, C
Hara, T
Hayakawa, T
Hollnagel, A
Ishiguro, K
Iuliano, A
Jakovcic, K
Jollet, C
Kamiscioglu, C
Kamiscioglu, M
Kim, S
Kitagawa, N
Klicek, B
Kodama, K
Komatsu, M
Kose, U
Kreslo, I
Laudisio, F
Lauria, A
Longhin, A
Loverre, P
Malgin, A
Mandrioli, G
Matsuo, T
Matveev, V
Mauri, N
Medinaceli, E
Meregaglia, A
Mikado, S
Miyanishi, M
Mizutani, F
Monacelli, P
Montesi, M
Morishima, K
Muciaccia, M
Naganawa, N
Naka, T
Nakamura, M
Nakano, T
Niwa, K
Ogawa, S
Okateva, N
Ozaki, K
Paoloni, A
Paparella, L
Park, B
Pasqualini, L
Pastore, A
Patrizii, L
Pessard, H
Podgrudkov, D
Polukhina, N
Pozzato, M
Pupilli, F
Roda, M
Roganova, T
Rokujo, H
Rosa, G
Ryazhskaya, O
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
Stipcevic, M
Strolin, P
Takahashi, S
Tenti, M
Terranova, F
Tioukov, V
Tufanli, S
Vasina, S
Vilain, P
Voevodina, E
Votano, L
Vuilleumier, J
Wilquet, G
Yoon, C
Agafonova N.
Alexandrov A.
Anokhina A.
Aoki S.
Ariga A.
Ariga T.
Bertolin A.
Bozza C.
Brugnera R.
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.
Fini R.A.
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.
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.
Okateva N.
Ozaki K.
Paoloni A.
Paparella L.
Park B.D.
Pasqualini L.
Pastore A.
Patrizii L.
Pessard H.
Podgrudkov D.
Polukhina N.
Pozzato M.
Pupilli F.
Roda M.
Roganova T.
Rokujo H.
Rosa G.
Ryazhskaya O.
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.
Vasina S.
Vilain P.
Voevodina E.
Votano L.
Vuilleumier J.L.
Wilquet G.
Yoon C.S.
Laboratoire d'Annecy de Physique des Particules (LAPP)
Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)
Source :
Phys.Rev.D, Phys.Rev.D, 2019, 100 (5), pp.051301. ⟨10.1103/PhysRevD.100.051301⟩, Physical Review D, Physical Review, PHYSICAL REVIEW D
Publication Year :
2019

Abstract

The OPERA experiment has conclusively observed the appearance of tau neutrinos in the muon neutrino CNGS beam. Exploiting the OPERA detector capabilities, it was possible to isolate high purity samples of $\nu_{e}$, $\nu_{\mu}$ and $\nu_{\tau}$ charged current weak neutrino interactions, as well as neutral current weak interactions. In this Letter, the full dataset is used for the first time to test the three-flavor neutrino oscillation model and to derive constraints on the existence of a light sterile neutrino within the framework of the $3+1$ neutrino model. For the first time, tau and electron neutrino appearance channels are jointly used to test the sterile neutrino hypothesis. A significant fraction of the sterile neutrino parameter space allowed by LSND and MiniBooNE experiments is excluded at 90% C.L. In particular, the best-fit values obtained by MiniBooNE combining neutrino and antineutrino data are excluded at 3.3 $\sigma$ significance.<br />Comment: 7 pages, 4 figures; Editors: Budimir Kli\v{c}ek and Matteo Tenti

Details

Language :
English
Database :
OpenAIRE
Journal :
Phys.Rev.D, Phys.Rev.D, 2019, 100 (5), pp.051301. ⟨10.1103/PhysRevD.100.051301⟩, Physical Review D, Physical Review, PHYSICAL REVIEW D
Accession number :
edsair.doi.dedup.....4c36dff34dd0f5dc41ee386fc46c6674
Full Text :
https://doi.org/10.1103/PhysRevD.100.051301⟩