NPAC (Nuclear/Particle/Astro/Cosmo) Forums |
Organized by: Prof. Lu Lu
U(1)' models. Unlike the usual wisdom, a spontaneous CP violation
plays a key role in this picture. This makes the EWBG in the U(1)'
models be very different from what happens in the minimal
supersymmetric standard model. I will also show that a successful
EWBG and an acceptable neutralino dark matter relic density can be
simultaneously achieved in our models.