The OPERA experiment is designed to search for nu(mu) -> nu(tau) oscillations in appearance mode, i.e., through the direct observation of the tau lepton in nu(tau)- charged current interactions. The experiment has taken data for five years, since 2008, with the CERN Neutrino to Gran Sasso beam. Previously, two nu(tau) candidates with a t decaying into hadrons were observed in a subsample of data of the 2008-2011 runs. Here we report the observation of a third nu(tau) candidate in the tau(-) -> mu(-) decay channel coming from the analysis of a subsample of the 2012 run. Taking into account the estimated background, the absence of nu(mu) -> nu(tau) oscillations is excluded at the 3.4 sigma level.

Evidence for nu(mu) -> nu(tau) appearance in the CNGS neutrino beam with the OPERA experiment / N. Agafonova;A. Aleksandrov;A. Anokhina;S. Aoki;A. Ariga;T. Ariga;T. Asada;D. Autiero;A. B. Dhahbi;A. Badertscher;D. Bender;A. Bertolin;C. Bozza;R. Brugnera;F. Brunet;G. Brunetti;A. Buonaura;S. Buontempo;B. Buettner;L. Chaussard;M. Chernyavsky;V. Chiarella;A. Chukanov;L. Consiglio;N. D'Ambrosio;G. D. Lellis;M. D. Serio;P. D. Amo;A. D. Crescenzo;D. D. Ferdinando;N. D. Marco;S. Dmitrievski;M. Dracos;D. Duchesneau;S. Dusini;T. Dzhatdoev;J. Ebert;A. Ereditato;J. Favier;T. Ferber;G. Ferone;R. A. Fini;T. Fukuda;G. Galati;A. Garfagnini;G. Giacomelli;C. Goellnitz;J. Goldberg;Y. Gornushkin;G. Grella;F. Grianti;M. Guler;C. Gustavino;C. Hagner;K. Hakamata;T. Hara;T. Hayakawa;M. Hierholzer;A. Hollnagel;B. Hosseini;H. Ishida;K. Ishiguro;M. Ishikawa;K. Jakovcic;C. Jollet;C. Kamiscioglu;M. Kamiscioglu;T. Katsuragawa;J. Kawada;H. Kawahara;J. H. Kim;S. H. Kim;M. Kimura;N. Kitagawa;B. Klicek;K. Kodama;M. Komatsu;U. Kose;I. Kreslo;A. Lauria;J. Lenkeit;A. Ljubicic;A. Longhin;P. Loverre;A. Malgin;G. Mandrioli;J. Marteau;T. Matsuo;V. Matveev;N. Mauri;E. Medinaceli;A. Meregaglia;P. Migliozzi;S. Mikado;M. Miyanishi;E. Miyashita;P. Monacelli;M. C. Montesi;K. Morishima;M. T. Muciaccia;N. Naganawa;T. Naka;M. Nakamura;T. Nakano;Y. Nakatsuka;K. Niwa;S. Ogawa;N. Okateva;A. Olshevsky;T. Omura;K. Ozaki;A. Paoloni;B. D. Park;I. G. Park;A. Pastore;L. Patrizii;E. Pennacchio;H. Pessard;C. Pistillo;D. Podgrudkov;N. Polukhina;M. Pozzato;K. Pretzl;F. Pupilli;R. Rescigno;M. Roda;H. Rokujo;T. Roganova;G. Rosa;I. Rostovtseva;A. Rubbia;O. Ryazhskaya;O. Sato;Y. Sato;A. Schembri;W. Schmidt-Parzefal;I. Shakiryanova;T. Shchedrina;A. Sheshukov;H. Shibuya;T. Shiraishi;G. Shoziyoev;S. Simone;M. Sioli;C. Sirignano;G. Sirri;M. Spinetti;L. Stanco;N. Starkov;S. M. Stellacci;M. Stipcevic;T. Strauss;P. Strolin;K. Suzuki;S. Takahashi;M. Tenti;F. Terranova;V. Tioukov;S. Tufanli;P. Vilain;M. Vladimirov;L. Votano;J. L. Vuilleumier;G. Wilquet;B. Wonsak;C. S. Yoon;J. Yoshida;M. Yoshimoto;Y. Zaitsev;S. Zemskova;A. Zghiche. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 89:(2014), pp. 051102-1-051102-6. [10.1103/PhysRevD.89.051102]

Evidence for nu(mu) -> nu(tau) appearance in the CNGS neutrino beam with the OPERA experiment

MAURI, NICOLETTA;MEDINACELI VILLEGAS, EDUARDO;POZZATO, MICHELE;SIOLI, MAXIMILIANO;SIRRI, GABRIELE;TENTI, MATTEO;
2014

Abstract

The OPERA experiment is designed to search for nu(mu) -> nu(tau) oscillations in appearance mode, i.e., through the direct observation of the tau lepton in nu(tau)- charged current interactions. The experiment has taken data for five years, since 2008, with the CERN Neutrino to Gran Sasso beam. Previously, two nu(tau) candidates with a t decaying into hadrons were observed in a subsample of data of the 2008-2011 runs. Here we report the observation of a third nu(tau) candidate in the tau(-) -> mu(-) decay channel coming from the analysis of a subsample of the 2012 run. Taking into account the estimated background, the absence of nu(mu) -> nu(tau) oscillations is excluded at the 3.4 sigma level.
2014
Evidence for nu(mu) -> nu(tau) appearance in the CNGS neutrino beam with the OPERA experiment / N. Agafonova;A. Aleksandrov;A. Anokhina;S. Aoki;A. Ariga;T. Ariga;T. Asada;D. Autiero;A. B. Dhahbi;A. Badertscher;D. Bender;A. Bertolin;C. Bozza;R. Brugnera;F. Brunet;G. Brunetti;A. Buonaura;S. Buontempo;B. Buettner;L. Chaussard;M. Chernyavsky;V. Chiarella;A. Chukanov;L. Consiglio;N. D'Ambrosio;G. D. Lellis;M. D. Serio;P. D. Amo;A. D. Crescenzo;D. D. Ferdinando;N. D. Marco;S. Dmitrievski;M. Dracos;D. Duchesneau;S. Dusini;T. Dzhatdoev;J. Ebert;A. Ereditato;J. Favier;T. Ferber;G. Ferone;R. A. Fini;T. Fukuda;G. Galati;A. Garfagnini;G. Giacomelli;C. Goellnitz;J. Goldberg;Y. Gornushkin;G. Grella;F. Grianti;M. Guler;C. Gustavino;C. Hagner;K. Hakamata;T. Hara;T. Hayakawa;M. Hierholzer;A. Hollnagel;B. Hosseini;H. Ishida;K. Ishiguro;M. Ishikawa;K. Jakovcic;C. Jollet;C. Kamiscioglu;M. Kamiscioglu;T. Katsuragawa;J. Kawada;H. Kawahara;J. H. Kim;S. H. Kim;M. Kimura;N. Kitagawa;B. Klicek;K. Kodama;M. Komatsu;U. Kose;I. Kreslo;A. Lauria;J. Lenkeit;A. Ljubicic;A. Longhin;P. Loverre;A. Malgin;G. Mandrioli;J. Marteau;T. Matsuo;V. Matveev;N. Mauri;E. Medinaceli;A. Meregaglia;P. Migliozzi;S. Mikado;M. Miyanishi;E. Miyashita;P. Monacelli;M. C. Montesi;K. Morishima;M. T. Muciaccia;N. Naganawa;T. Naka;M. Nakamura;T. Nakano;Y. Nakatsuka;K. Niwa;S. Ogawa;N. Okateva;A. Olshevsky;T. Omura;K. Ozaki;A. Paoloni;B. D. Park;I. G. Park;A. Pastore;L. Patrizii;E. Pennacchio;H. Pessard;C. Pistillo;D. Podgrudkov;N. Polukhina;M. Pozzato;K. Pretzl;F. Pupilli;R. Rescigno;M. Roda;H. Rokujo;T. Roganova;G. Rosa;I. Rostovtseva;A. Rubbia;O. Ryazhskaya;O. Sato;Y. Sato;A. Schembri;W. Schmidt-Parzefal;I. Shakiryanova;T. Shchedrina;A. Sheshukov;H. Shibuya;T. Shiraishi;G. Shoziyoev;S. Simone;M. Sioli;C. Sirignano;G. Sirri;M. Spinetti;L. Stanco;N. Starkov;S. M. Stellacci;M. Stipcevic;T. Strauss;P. Strolin;K. Suzuki;S. Takahashi;M. Tenti;F. Terranova;V. Tioukov;S. Tufanli;P. Vilain;M. Vladimirov;L. Votano;J. L. Vuilleumier;G. Wilquet;B. Wonsak;C. S. Yoon;J. Yoshida;M. Yoshimoto;Y. Zaitsev;S. Zemskova;A. Zghiche. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 89:(2014), pp. 051102-1-051102-6. [10.1103/PhysRevD.89.051102]
N. Agafonova;A. Aleksandrov;A. Anokhina;S. Aoki;A. Ariga;T. Ariga;T. Asada;D. Autiero;A. B. Dhahbi;A. Badertscher;D. Bender;A. Bertolin;C. Bozza;R. Brugnera;F. Brunet;G. Brunetti;A. Buonaura;S. Buontempo;B. Buettner;L. Chaussard;M. Chernyavsky;V. Chiarella;A. Chukanov;L. Consiglio;N. D'Ambrosio;G. D. Lellis;M. D. Serio;P. D. Amo;A. D. Crescenzo;D. D. Ferdinando;N. D. Marco;S. Dmitrievski;M. Dracos;D. Duchesneau;S. Dusini;T. Dzhatdoev;J. Ebert;A. Ereditato;J. Favier;T. Ferber;G. Ferone;R. A. Fini;T. Fukuda;G. Galati;A. Garfagnini;G. Giacomelli;C. Goellnitz;J. Goldberg;Y. Gornushkin;G. Grella;F. Grianti;M. Guler;C. Gustavino;C. Hagner;K. Hakamata;T. Hara;T. Hayakawa;M. Hierholzer;A. Hollnagel;B. Hosseini;H. Ishida;K. Ishiguro;M. Ishikawa;K. Jakovcic;C. Jollet;C. Kamiscioglu;M. Kamiscioglu;T. Katsuragawa;J. Kawada;H. Kawahara;J. H. Kim;S. H. Kim;M. Kimura;N. Kitagawa;B. Klicek;K. Kodama;M. Komatsu;U. Kose;I. Kreslo;A. Lauria;J. Lenkeit;A. Ljubicic;A. Longhin;P. Loverre;A. Malgin;G. Mandrioli;J. Marteau;T. Matsuo;V. Matveev;N. Mauri;E. Medinaceli;A. Meregaglia;P. Migliozzi;S. Mikado;M. Miyanishi;E. Miyashita;P. Monacelli;M. C. Montesi;K. Morishima;M. T. Muciaccia;N. Naganawa;T. Naka;M. Nakamura;T. Nakano;Y. Nakatsuka;K. Niwa;S. Ogawa;N. Okateva;A. Olshevsky;T. Omura;K. Ozaki;A. Paoloni;B. D. Park;I. G. Park;A. Pastore;L. Patrizii;E. Pennacchio;H. Pessard;C. Pistillo;D. Podgrudkov;N. Polukhina;M. Pozzato;K. Pretzl;F. Pupilli;R. Rescigno;M. Roda;H. Rokujo;T. Roganova;G. Rosa;I. Rostovtseva;A. Rubbia;O. Ryazhskaya;O. Sato;Y. Sato;A. Schembri;W. Schmidt-Parzefal;I. Shakiryanova;T. Shchedrina;A. Sheshukov;H. Shibuya;T. Shiraishi;G. Shoziyoev;S. Simone;M. Sioli;C. Sirignano;G. Sirri;M. Spinetti;L. Stanco;N. Starkov;S. M. Stellacci;M. Stipcevic;T. Strauss;P. Strolin;K. Suzuki;S. Takahashi;M. Tenti;F. Terranova;V. Tioukov;S. Tufanli;P. Vilain;M. Vladimirov;L. Votano;J. L. Vuilleumier;G. Wilquet;B. Wonsak;C. S. Yoon;J. Yoshida;M. Yoshimoto;Y. Zaitsev;S. Zemskova;A. Zghiche
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/374662
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