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Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment

The OPERA experiment is aiming at the first direct detection of neutrino oscillations in appearance mode through the study of the {\nu}{\mu} {\tp} {\nu}{\tau} channel. The OPERA detector is placed in the CNGS long baseline {\nu}{\mu} beam 730 km away from the neutrino source. The analysis of a sub-s...

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Detalles Bibliográficos
Autor principal: Esposito, L.S.
Lenguaje:eng
Publicado: 2011
Materias:
Acceso en línea:http://cds.cern.ch/record/1354052
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author Esposito, L.S.
author_facet Esposito, L.S.
author_sort Esposito, L.S.
collection CERN
description The OPERA experiment is aiming at the first direct detection of neutrino oscillations in appearance mode through the study of the {\nu}{\mu} {\tp} {\nu}{\tau} channel. The OPERA detector is placed in the CNGS long baseline {\nu}{\mu} beam 730 km away from the neutrino source. The analysis of a sub-sample of the data taken in the 2008-2009 runs was completed. After a brief description of the beam and the experimental setup, we report on event analysis and on a first candidate event, its background estimation and statistical significance.
id cern-1354052
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2011
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spelling cern-13540522019-09-30T06:29:59Zhttp://cds.cern.ch/record/1354052engEsposito, L.S.Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experimentParticle Physics - ExperimentThe OPERA experiment is aiming at the first direct detection of neutrino oscillations in appearance mode through the study of the {\nu}{\mu} {\tp} {\nu}{\tau} channel. The OPERA detector is placed in the CNGS long baseline {\nu}{\mu} beam 730 km away from the neutrino source. The analysis of a sub-sample of the data taken in the 2008-2009 runs was completed. After a brief description of the beam and the experimental setup, we report on event analysis and on a first candidate event, its background estimation and statistical significance.The OPERA experiment is aiming at the first direct detection of neutrino oscillations in appearance mode through the study of the {\nu}{\mu} {\tp} {\nu}{\tau} channel. The OPERA detector is placed in the CNGS long baseline {\nu}{\mu} beam 730 km away from the neutrino source. The analysis of a sub-sample of the data taken in the 2008-2009 runs was completed. After a brief description of the beam and the experimental setup, we report on event analysis and on a first candidate event, its background estimation and statistical significance.arXiv:1105.5239oai:cds.cern.ch:13540522011-05-27
spellingShingle Particle Physics - Experiment
Esposito, L.S.
Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title_full Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title_fullStr Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title_full_unstemmed Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title_short Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment
title_sort search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the opera experiment
topic Particle Physics - Experiment
url http://cds.cern.ch/record/1354052
work_keys_str_mv AT espositols searchfornumutonutauoscillationsinappearancemodeintheoperaexperiment