Mass production (Super-K) Setup of jnubeam – 3 horn 250 kA – 30-GeV proton beam of Gaussian distribution ( x,y = 0.4243 cm) – On center, parallel beam.
Development of Cryogenic Tracking Detectors for Low-energy Solar Neutrinos
Whatever happened to Solar n ’s?
Neutrinos are tiny, neutral, elementary particles which interact with matter via the “weak force”. The Sun produces over two hundred trillion trillion.
