Analysis of information sources in references of the Wikipedia article "中微子" in Chinese language version.
The rate of interaction of electron neutrino, muon neutrino, tau neutrino, muon antineutrino, tau antineutrino, with electron is mostly negligible compared to interactions with nucleons. However, the case of electron antineutrino is unique because of [Glashow resonance at energy of about 6.3 PeV]
The detector consists of a 12 m diameter acrylic sphere containing 1000 tonnes of heavy water...[Solar neutrinos] are detected at SNO via the charged current process of electron neutrinos interacting with deuterons to produce two protons and an electron
The rate of interaction of electron neutrino, muon neutrino, tau neutrino, muon antineutrino, tau antineutrino, with electron is mostly negligible compared to interactions with nucleons. However, the case of electron antineutrino is unique because of [Glashow resonance at energy of about 6.3 PeV]
In 1989, experimenters at CERN found proof that the tau neutrino is the third and last light neutrino of the Standard Model, but a direct observation was not yet feasible.
The central detector, in which the antineutrinos are detected, consists of four stainless-steel cells filled with a cubic meter of liquid scintillator. The scintillator contains plenty of quasi-free protons and is laced with gadolinium atoms.
That group found, although with less precision, that the neutrino speeds were consistent with the speed of light.
In 1989, experimenters at CERN found proof that the tau neutrino is the third and last light neutrino of the Standard Model, but a direct observation was not yet feasible.
The central detector, in which the antineutrinos are detected, consists of four stainless-steel cells filled with a cubic meter of liquid scintillator. The scintillator contains plenty of quasi-free protons and is laced with gadolinium atoms.
The detector consists of a 12 m diameter acrylic sphere containing 1000 tonnes of heavy water...[Solar neutrinos] are detected at SNO via the charged current process of electron neutrinos interacting with deuterons to produce two protons and an electron
The rate of interaction of electron neutrino, muon neutrino, tau neutrino, muon antineutrino, tau antineutrino, with electron is mostly negligible compared to interactions with nucleons. However, the case of electron antineutrino is unique because of [Glashow resonance at energy of about 6.3 PeV]
That group found, although with less precision, that the neutrino speeds were consistent with the speed of light.