New Journal of Physics · 2006 · 101 citations · 28 references
The OPERA neutrino detector at the underground Gran Sasso \nLaboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode, through the study of νμ → ντ oscillations. The apparatus consists of a lead/emulsion-film target complemented by electronic detectors. It is placed in the high-energy, long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. In August 2006, a first run with \nCNGS neutrinos was successfully conducted. A first sample of neutrino events was collected, statistically consistent with the integrated beam intensity. After a brief description of the beam and of the various sub-detectors, we report on the achievement of this milestone, presenting the first data and some analysis results.
28
Evidence for Oscillation of Atmospheric Neutrinos
Y. Fukuda, T. Hayakawa, E. Ichihara et al. · Physical Review Letters · 1998 · 4.8K citations · Full text
Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days
Y. Fukuda, T. Hayakawa, E. Ichihara et al. · Physical Review Letters · 1998 · 720 citations · Full text