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تسجيل مستخدم جديدEvidence for $ u_mu to u_tau$ appearance in the CNGS neutrino beam with the OPERA experiment
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The OPERA experiment is designed to search for $ u_{mu} rightarrow u_{tau}$ oscillations in appearance mode i.e. through the direct observation of the $tau$ lepton in $ u_{tau}$ charged current interactions. The experiment has taken data for five years, since 2008, with the CERN Neutrino to Gran Sasso beam. Previously, two $ u_{tau}$ candidates with a $tau$ decaying into hadrons were observed in a sub-sample of data of the 2008-2011 runs. Here we report the observation of a third $ u_tau$ candidate in the $tau^-tomu^-$ decay channel coming from the analysis of a sub-sample of the 2012 run. Taking into account the estimated background, the absence of $ u_{mu} rightarrow u_{tau}$ oscillations is excluded at the 3.4 $sigma$ level.
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The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the $ u_mu to u_tau$ channel, via the detection of the $tau$-leptons created in charged current $ u_tau$ interactions. T
he detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17 GeV. The observation of the first $ u_tau$ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional $ u_tau$ candidate has been observed. The significance of the two events in terms of a $ u_mu to u_tau$ oscillation signal is of 2.40 $sigma$.
OPERA is a long-baseline experiment designed to search for $ u_{mu}to u_{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 dis
covery of $ u_tau$ appearance in 2015, with $5.1sigma$ significance, the criteria to select $ u_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 $ u_tau$ properties has been improved. Results are reported.
The OPERA experiment was designed to study $ u_muto u_tau$ oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to $17.97cdot 10^
{19}$ protons on target. Selection criteria looser than in previous analyses have produced ten $ u_tau$ candidate events, thus reducing the statistical uncertainty in the measurement of the oscillation parameters and of $ u_tau$ properties. A multivariate approach for event identification has been applied to the candidate events and the discovery of $ u_tau$ appearance is confirmed with an improved significance level of 6.1 $sigma$. $Delta m^2_{23}$ has been measured, in appearance mode, with an accuracy of 20%. The measurement of $ u_tau$ CC cross-section, for the first time with a negligible contamination from $bar{ u}_tau$, and the first direct observation of the $ u_tau$ lepton number are also reported.
The OPERA experiment was designed to search for $ u_{mu} rightarrow u_{tau}$ oscillations in appearance mode, i.e. by detecting the $tau$-leptons produced in charged current $ u_{tau}$ interactions. The experiment took data from 2008 to 2012 in the
CERN Neutrinos to Gran Sasso beam. The observation of $ u_{mu} rightarrow u_{tau}$ appearance, achieved with four candidate events in a sub-sample of the data, was previously reported. In this paper, a fifth $ u_{tau}$ 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 assessing the discovery of $ u_{mu}rightarrow u_{tau}$ oscillations in appearance mode with a significance larger than 5 $sigma$.
The OPERA experiment in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode in the muon neutrino to tau neutrino channel. The detector is hybrid, being made
of an emulsion/lead target and of electronic detectors. It is placed in the CNGS neutrino beam 730 km away from the neutrino source. Runs with CNGS neutrinos were successfully carried out in 2008, 2009, and 2010. After a brief description of the beam and the experimental setup, we report on event analysis of a sample of events corresponding to 1.89times 10^{19} p.o.t. in the CERN CNGS u_{mu} beam that yielded the observation of a first candidate u_{tau} CC interaction. The topology and kinematics of this candidate event are described in detail. The background sources are explained and the significance of the candidate is assessed.
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