ELECTRON TO TAU-NEUTRINO OSCILLATIONS

1993 ◽  
Author(s):  
GIANNI CONFORTO
Keyword(s):  
Neutrino Oscillations ◽  
Tau Neutrino

Search for tau-neutrino oscillations at CERN

1996 ◽  
Vol 109 (6-7) ◽  
pp. 951-956
Author(s):  
G. Piredda
Keyword(s):  
Neutrino Oscillations ◽  
Tau Neutrino

scholarly journals Dataset of tau neutrino interactions recorded by the OPERA experiment

2020 ◽  
Vol 245 ◽  
pp. 08013
Author(s):  
Giovanni De Lellis ◽  
Sergey Dmitrievsky ◽  
Giuliana Galati ◽  
Artemis Lavasa ◽  
Tibor Šimko ◽  
...  
Keyword(s):  
Neutrino Oscillations ◽  
Rare Events ◽  
Open Data ◽  
Muon Neutrinos ◽  
Tau Neutrino ◽  
Neutrino Interactions ◽  
Visualisation Tool ◽  
Data Release ◽  
Data Portal

We describe the dataset of very rare events recorded by the OPERA experiment. The events represent tracks of particles associated with tau neutrino interactions coming from the transformation of muon neutrinos due to a process known as neutrino oscillations. The events have been published on the CERN Open Data Portal. We describe the dataset semantics and the interactive event display visualisation tool accompanying the data release.

scholarly journals ATMOSPHERIC AND GALACTIC TAU NEUTRINOS

2004 ◽  
Vol 19 (13n16) ◽  
pp. 1171-1178 ◽  
Author(s):  
H. ATHAR
Keyword(s):  
Lower Energy ◽  
Neutrino Oscillations ◽  
Galactic Plane ◽  
Neutrino Flux ◽  
Earth Atmosphere ◽  
Future Prospects ◽  
Energy Value ◽  
Tau Neutrino ◽  
Tau Neutrinos ◽  
The Earth

Neutrinos with energy greater than GeV are copiously produced in the p(A,p) interactions occurring in the earth atmosphere and in our galactic plane. A comparison of the tau and mu neutrino flux in the presence of neutrino oscillations from these two astrophysical sites is presented. It is pointed out that the galactic plane tau neutrino flux dominates over the downward going atmospheric tau neutrino flux at much lower energy value than that for the dominance of the mu neutrino flux from these two sites. Future prospects for possible observations of galactic tau neutrino flux are also briefly mentioned.

scholarly journals OPERA tau neutrino charged current interactions

2021 ◽  
Vol 8 (1) ◽  
Author(s):  
N. Agafonova ◽  
A. Alexandrov ◽  
A. Anokhina ◽  
S. Aoki ◽  
A. Ariga ◽  
...  
Keyword(s):  
Neutrino Oscillations ◽  
Statistical Significance ◽  
Open Data ◽  
Photographic Emulsion ◽  
Charged Current ◽  
Lead Target ◽  
Tau Neutrino ◽  
Data Portal

AbstractThe OPERA experiment was designed to discover the vτ appearance in a vμ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. It was exposed from 2008 to 2012 to the CNGS beam: an almost pure vμ beam with a baseline of 730 km, collecting a total of 1.8·1020 protons on target. The OPERA Collaboration eventually assessed the discovery of vμ→vτ oscillations with a statistical significance of 6.1 σ by observing ten vτ CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a detailed description of the vτ data sample to make it usable by the whole community.

scholarly journals CONFRONTING HEAVY TAU NEUTRINOS WITH NEUTRINO OSCILLATIONS

2001 ◽  
Vol 16 (26) ◽  
pp. 1699-1702 ◽  
Author(s):  
CHUN LIU
Keyword(s):  
Neutrino Mass ◽  
Neutrino Oscillations ◽  
Electron Neutrino ◽  
Supersymmetric Model ◽  
Tau Neutrino ◽  
Tau Neutrinos ◽  
Mass Pattern

If the tau neutrino is as heavy as 10 MeV which may have certain astrophysical implications, the neutrino mass pattern is studied so as to accommodate the new oscillation observations. It predicts that the electron neutrino has Marjorana mass around 0.05 eV. A supersymmetric model is described to realize the above scenario.

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