One phenomenon predicted by this theory was a leptonic muon antineutrino-electron scattering event detected in the Gargamelle bubble chamber. One parameter predicted by this theory has a sine-squared value of 0.23, and this theory predicts the behavior of the universe in a namesake epoch with energy greater than 100 GeV. Another prediction of this theory was confirmed by the UA1 experiment, which used stochastic cooling and won Carlo Rubbia and Simon (*) van der Meer the Nobel. Veltman and t'Hooft showed that this theory was renormalizable, and this theory predicts the
One phenomenon predicted by this theory was a leptonic muon antineutrino-electron scattering event detected in the Gargamelle bubble chamber. One parameter predicted by this theory has a sine-squared value of 0.23, and this theory predicts the behavior of the universe in a namesake epoch with energy greater than 100 GeV. Another prediction of this theory was confirmed by the UA1 experiment, which used stochastic cooling and won Carlo Rubbia and Simon (*) van der Meer the Nobel. Veltman and t'Hooft showed that this theory was renormalizable, and this theory predicts the existence of neutral currents. The Higgs mechanism is responsible for breaking this theory's SU(2) x U(1) gauge symmetry, which causes three of the four vector bosons it posits to acquire a positive mass; those three massive particles are the W-plus, W-minus, and Z. Originally posited by Glashow, Weinberg, and Salam, for 10 points, name this theory which unifies two of the four fundamental forces.
One phenomenon predicted by this theory was a leptonic muon antineutrino-electron scattering event detected in the Gargamelle bubble chamber.
electroweak [accept Glashow-Weinberg-Salam theory until mention]