| Budget Amount *help |
¥2,200,000 (Direct Cost: ¥2,200,000)
Fiscal Year 1995: ¥500,000 (Direct Cost: ¥500,000)
Fiscal Year 1994: ¥500,000 (Direct Cost: ¥500,000)
Fiscal Year 1993: ¥1,200,000 (Direct Cost: ¥1,200,000)
|
|---|
| Research Abstract |
1. Effects of the heavy neutrino in the 4th generation have been investigated in the e^+e^---> W^+W^- process, where 1) weak boson's 3 point formfactors, 2) differential cross sections, and 3) foreward-backward asymmetry was estimated. It has been shown that the neutrino type of Majorana or Dirac can be determined from the "threshold behavior of the scattering amplitudes", When the polarizd electron and positron beams are adopted as well as the polarization measurement of the final W' s can be performed. In the next collider energies the the heavy neutrinos' contibution to the cross sections is about 0.5%. 2. Baryogenesis at electoroweak scale has been studies using the heavy neutrinos. The lepton number generation rate has been estimated from the scattering of the neutrinos from the bubbles which appear in the development of the lstorder phase transition of our universe. Furthermore, simulation has been performed including the generation, fusion and growth effects of the bubbles, leading to the 2-3 times larger value for the produced to tallepton numbers. The observed value of the baryon number can be explained with the 100GeV and 50 GeV neutrinos at the phase transition temperature of 100K.3. CP violation effects in the weak boson's pair production processes have been studied in the model (1) with the heavy vector-like down-type quark, leading to the small value of 10^<-9>. In the supersymmetric standard model (2), however, a rather big value of 10^<-(4-5)> has been found due to the extra CP violationin the softly susy breaking term. 4. As the other baryogenesis model, the hyper-charge generation rate has been estimated in the presence of the up-type vector-like quark of 500 GeV,and the phase transition dynamics has been studied in this model. 5. Atmospheric neutrino problem has been examined in the 3 generation model of the neutrino oscillation.
|
