Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam

The sensitivity of the present CNGS beam to the sub-dominant $\nu_\mu \leftrightarrow \nu_e$ oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to $\theta_{13}$ o...

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Detalles Bibliográficos
Autores principales: Komatsu, M, Migliozzi, P, Terranova, F
Lenguaje:eng
Publicado: 2002
Materias:
Detectors and Experimental Techniques
Acceso en línea:https://dx.doi.org/10.1088/0954-3899/29/2/318
http://cds.cern.ch/record/584398
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author Komatsu, M
Migliozzi, P
Terranova, F
author_facet Komatsu, M
Migliozzi, P
Terranova, F
author_sort Komatsu, M
collection CERN
description The sensitivity of the present CNGS beam to the sub-dominant $\nu_\mu \leftrightarrow \nu_e$ oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to $\theta_{13}$ of ICARUS and OPERA combined. We show that the CNGS beam optimised for $\nu_\tau$ appearance, will improve significantly (about a factor 5) the current limit of CHOOZ and explore most of the region $\sin^22\theta_{13}\simeq\mathcal{O}(10^{-2})$.
id cern-584398
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
record_format invenio
spelling cern-5843982019-09-30T06:29:59Zdoi:10.1088/0954-3899/29/2/318http://cds.cern.ch/record/584398engKomatsu, MMigliozzi, PTerranova, FSensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beamDetectors and Experimental TechniquesThe sensitivity of the present CNGS beam to the sub-dominant $\nu_\mu \leftrightarrow \nu_e$ oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to $\theta_{13}$ of ICARUS and OPERA combined. We show that the CNGS beam optimised for $\nu_\tau$ appearance, will improve significantly (about a factor 5) the current limit of CHOOZ and explore most of the region $\sin^22\theta_{13}\simeq\mathcal{O}(10^{-2})$.hep-ph/0210043oai:cds.cern.ch:5843982002-10-02
spellingShingle Detectors and Experimental Techniques
Komatsu, M
Migliozzi, P
Terranova, F
Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title_full Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title_fullStr Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title_full_unstemmed Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title_short Sensitivity to $\theta_{13}$ of the CERN to Gran Sasso neutrino beam
title_sort sensitivity to $\theta_{13}$ of the cern to gran sasso neutrino beam
topic Detectors and Experimental Techniques
url https://dx.doi.org/10.1088/0954-3899/29/2/318
http://cds.cern.ch/record/584398
work_keys_str_mv AT komatsum sensitivitytotheta13ofthecerntogransassoneutrinobeam
AT migliozzip sensitivitytotheta13ofthecerntogransassoneutrinobeam
AT terranovaf sensitivitytotheta13ofthecerntogransassoneutrinobeam

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