Their interaction with a neutron results in the exchange of a W minus particle, thus producing a proton, and they were detected in radiation from Supernova 1987A by the Super Kamiokande reactor.
Their interaction with a neutron results in the exchange of a W minus particle, thus producing a proton, and they were detected in radiation from Supernova 1987A by the Super Kamiokande reactor. Their existence was proposed by Wolfgang Pauli, to account for the missing energy during a beta decay process, and they exist in muon, tau, and electron varieties. Represented by the letter nu, for 10 points, identify these uncharged particles known for having a very high velocity and a low mass.
Their interaction with a neutron results in the exchange of a W minus particle, thus producing a proton, and they were detected in radiation from Supernova 1987A by the Super Kamiokande reactor.
neutrinos