The OPERA experiment
Identifieur interne : 000823 ( France/Analysis ); précédent : 000822; suivant : 000824The OPERA experiment
Auteurs : C. Jollet [France]Source :
- Physics of Atomic Nuclei / Yadernaya Fizika [ 1063-7788 ] ; 2006.
Abstract
The aim of the OPERA experiment is to provide an unambiguous evidence for the νμ ↔ ντ oscillation by looking at the appearance of ντ in a pure νμ beam. This oscillation will be sought in the region of the oscillation parameters indicated by the atmospheric neutrino results. The experiment is part of the CNGS (Cern Neutrino beam to Gran Sasso) project. The νμ beam produced at CERN will be sent towards the Gran Sasso underground laboratory, where the OPERA detector is under construction. The detector, the physics potential and performance for neutrino oscillation studies including the subleading νμ ↔ νe search are presented.
Url:
Affiliations:
Links toward previous steps (curation, corpus...)
- to stream Hal, to step Corpus: 000269
- to stream Hal, to step Curation: 000269
- to stream Hal, to step Checkpoint: 000770
- to stream Main, to step Merge: 001A24
- to stream Main, to step Curation: 001984
- to stream Main, to step Exploration: 001984
- to stream France, to step Extraction: 000823
Links to Exploration step
Hal:in2p3-00118917Le document en format XML
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<front><div type="abstract" xml:lang="en">The aim of the OPERA experiment is to provide an unambiguous evidence for the νμ ↔ ντ oscillation by looking at the appearance of ντ in a pure νμ beam. This oscillation will be sought in the region of the oscillation parameters indicated by the atmospheric neutrino results. The experiment is part of the CNGS (Cern Neutrino beam to Gran Sasso) project. The νμ beam produced at CERN will be sent towards the Gran Sasso underground laboratory, where the OPERA detector is under construction. The detector, the physics potential and performance for neutrino oscillation studies including the subleading νμ ↔ νe search are presented.</div>
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