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The OPERA experiment: a direct search of the $\nu_\mu \longrightarrow \nu_\tau$ oscillations
High Energy Physics - Experiment · Submitted 19 Oct 2009
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim In this paper the detector and the analysis strategy are described and the status of the analysis of the 2008 and 2009 runs is discussed.
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The abstract, sentence by sentence
The aim of the OPERA experiment is to search for the appearance of the tau neutrino in the quasi pure muon neutrino beam produced at CERN (CNGS). The detector, installed in the Gran Sasso underground laboratory 730 km away from CERN, consists of a lead/emulsion target complemented with electronic detectors. After a short pilot run in 2007, a first physics run took place from June to November 2008. The second physics run started in June 2009. At present a total (2008+2009) of 4.2 10$^{19}$ protons on target were delivered by the CNGS, producing more than 25,000 events in time coincidence in the OPERA detector. Among them \~4000 events occured in the target of the detector. In this paper the detector and the analysis strategy are described and the status of the analysis of the 2008 and 2009 runs is discussed.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The aim of the OPERA experiment is to search for the appearance of the tau neutrino in the quasi pure muon neutrino beam produced at CERN (CNGS). | contribution 0.67 | 0.25 | 0.03 | asserted 0.90 |
| s1 | The detector, installed in the Gran Sasso underground laboratory 730 km away from CERN, consists of a lead/emulsion target complemented with electronic detectors. | method 1.00 | 0.45 | 0.02 | asserted 1.00 |
| s2 | After a short pilot run in 2007, a first physics run took place from June to November 2008. | method 0.90 | 0.73 | 0.02 | asserted 1.00 |
| s3 | The second physics run started in June 2009. | method 0.88 | 0.50 | 0.01 | asserted 1.00 |
| s4 | At present a total (2008+2009) of 4.2 10$^{19}$ protons on target were delivered by the CNGS, producing more than 25,000 events in time coincidence in the OPERA detector. | result 0.50 | 0.83 | 0.03 | asserted 1.00 |
| s5 | Among them \~4000 events occured in the target of the detector. | result 0.89 | 0.87 | 0.02 | asserted 1.00 |
| s6 | In this paper the detector and the analysis strategy are described and the status of the analysis of the 2008 and 2009 runs is discussed. | contribution 0.86 | 0.64 | 0.04 | asserted 0.91 |
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Original abstract
The aim of the OPERA experiment is to search for the appearance of the tau neutrino in the quasi pure muon neutrino beam produced at CERN (CNGS). The detector, installed in the Gran Sasso underground laboratory 730 km away from CERN, consists of a lead/emulsion target complemented with electronic detectors. After a short pilot run in 2007, a first physics run took place from June to November 2008. The second physics run started in June 2009. At present a total (2008+2009) of 4.2 10$^{19}$ protons on target were delivered by the CNGS, producing more than 25,000 events in time coincidence in the OPERA detector. Among them \~4000 events occured in the target of the detector. In this paper the detector and the analysis strategy are described and the status of the analysis of the 2008 and 2009 runs is discussed.
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Cites as background 1 paper
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The major experimental results for solar [ref] , atmospheric [ref] , reactor [ref] or accelerator [ref] neutrinos were obtained by observing the “disappearance" of neutrinos wrt to a close position measurement or a predicted flux.
Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam · Introduction · 0.98
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