The OPERA experiment was designed to search for νμ → ντ oscillations in appearance mode, i.e., by detecting the τ leptons produced in charged current ντ interactions. The experiment took data from 2008 to 2012 in the CERN Neutrinos to Gran Sasso beam. The observation of the νμ → ντ appearance, achieved with four candidate events in a subsample of the data, was previously reported. In this Letter, a fifth ντ candidate event, found in an enlarged data sample, is described. Together with a further reduction of the expected background, the candidate events detected so far allow us to assess the discovery of νμ → ντ oscillations in appearance mode with a significance larger than 5σ.

Agafonova, N., Aleksandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., et al. (2015). Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment. PHYSICAL REVIEW LETTERS, 115(12), 1-7 [10.1103/PhysRevLett.115.121802].

Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment

DI FERDINANDO, DONATO;FORNARI, FEDERICO;MAURI, NICOLETTA;PASQUALINI, LAURA;PATRIZII, LAURA;POZZATO, MICHELE;SIOLI, MAXIMILIANO;SIRRI, GABRIELE;TENTI, MATTEO;
2015

Abstract

The OPERA experiment was designed to search for νμ → ντ oscillations in appearance mode, i.e., by detecting the τ leptons produced in charged current ντ interactions. The experiment took data from 2008 to 2012 in the CERN Neutrinos to Gran Sasso beam. The observation of the νμ → ντ appearance, achieved with four candidate events in a subsample of the data, was previously reported. In this Letter, a fifth ντ candidate event, found in an enlarged data sample, is described. Together with a further reduction of the expected background, the candidate events detected so far allow us to assess the discovery of νμ → ντ oscillations in appearance mode with a significance larger than 5σ.
2015
Agafonova, N., Aleksandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., et al. (2015). Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment. PHYSICAL REVIEW LETTERS, 115(12), 1-7 [10.1103/PhysRevLett.115.121802].
Agafonova, N; Aleksandrov, A.; Anokhina, A.; Aoki, S.; Ariga, A.; Ariga, T.; Bender, D.; Bertolin, A.; Bodnarchuk, I.; Bozza, C.; Brugnera, R.; Buonau...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/528611
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