Parity: from strong CP problem to dark matter, neutrino masses and baryon asymmetry
Abstract
We show that in an SU(3)c× [SU(2)L× U(1)Y]× [SU(2)'R× U(1)'Y] framework, the parity symmetry motivated by solving the strong CP problem without resorting to an axion can predict a dark matter particle with a mass around 302 GeV. This dark matter candidate can be directly detected in the presence of a U(1)Y× U(1)'Y kinetic mixing. Furthermore, our model can accommodate a natural way to simultaneously realize an inverse-linear seesaw for neutrino masses and a resonant leptogenesis for baryon asymmetry.
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