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Recent results of the OPERA experiment

The OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of ν<sub>τ</sub> in an almost pure ν<sub>μ</sub> beam (the CERN CNGS beam). In five years of physics run the experiment collected 17....

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Autor principal: Pupilli, Fabio
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1142/9789814603164_0044
http://cds.cern.ch/record/1645123
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author Pupilli, Fabio
author_facet Pupilli, Fabio
author_sort Pupilli, Fabio
collection CERN
description The OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of ν<sub>τ</sub> in an almost pure ν<sub>μ</sub> beam (the CERN CNGS beam). In five years of physics run the experiment collected 17.97 × 10<sup>19</sup> p.o.t. The detection of τS produced in ν<sub>τ</sub> CC interactions and of their decays is accomplished exploiting the high spatial resolution of nuclear emulsions. Furthermore OPERA has good capabilities in detecting electron neutrino interactions, setting limits on the ν<sub>μ</sub> → ν<sub>ℯ</sub> oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.
id cern-1645123
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
record_format invenio
spelling cern-16451232023-04-04T03:50:16Zdoi:10.1142/9789814603164_0044http://cds.cern.ch/record/1645123engPupilli, FabioRecent results of the OPERA experimentParticle Physics - ExperimentParticle Physics - ExperimentThe OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of ν<sub>τ</sub> in an almost pure ν<sub>μ</sub> beam (the CERN CNGS beam). In five years of physics run the experiment collected 17.97 × 10<sup>19</sup> p.o.t. The detection of τS produced in ν<sub>τ</sub> CC interactions and of their decays is accomplished exploiting the high spatial resolution of nuclear emulsions. Furthermore OPERA has good capabilities in detecting electron neutrino interactions, setting limits on the ν<sub>μ</sub> → ν<sub>ℯ</sub> oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.The OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of $\nu_{\tau}$ in an almost pure $\nu_{\mu}$ beam (the CERN CNGS beam). In five years of physics run the experiment collected $17.97 \times 10^{19}$ p.o.t. The detection of $\tau$s produced in $\nu_{\tau}$ CC interactions and of their decays is accomplished exploiting the high spatial resolution of nuclear emulsions. Furthermore OPERA has good capabilities in detecting electron neutrino interactions, setting limits on the $\nu_{\mu} \rightarrow \nu_{e}$ oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.arXiv:1401.6776oai:cds.cern.ch:16451232014-01-27
spellingShingle Particle Physics - Experiment
Particle Physics - Experiment
Pupilli, Fabio
Recent results of the OPERA experiment
title Recent results of the OPERA experiment
title_full Recent results of the OPERA experiment
title_fullStr Recent results of the OPERA experiment
title_full_unstemmed Recent results of the OPERA experiment
title_short Recent results of the OPERA experiment
title_sort recent results of the opera experiment
topic Particle Physics - Experiment
Particle Physics - Experiment
url https://dx.doi.org/10.1142/9789814603164_0044
http://cds.cern.ch/record/1645123
work_keys_str_mv AT pupillifabio recentresultsoftheoperaexperiment