Chiara Arina, Jinn-Ouk Gong, Narendra Sahu
We present a scalar triplet extension of the standard model to unify the origin of inflation with neutrino mass, asymmetric dark matter and leptogenesis. In presence of non-minimal couplings to gravity the scalar triplet, mixed with the standard model Higgs, plays the role of inflaton in the early Universe, while its decay to SM Higgs, lepton and dark matter simultaneously generate an asymmetry in the visible and dark matter sectors. On the other hand, in the low energy effective theory the induced vacuum expectation value of the triplet gives sub-eV Majorana masses to active neutrinos. We investigate the model parameter space leading to successful inflation as well as the observed dark matter to baryon abundance. Assuming the standard model like Higgs mass to be at 125 GeV, we show that the mass scale of the scalar triplet to be < O(10^8) GeV and the trilinear coupling of the triplet to doublet Higgs is < 0.09 in order to prevent vacuum instability at a scale < O(10^8) GeV. It is found that inflation strongly constrains the quartic couplings, while allowing for a wide range of Yukawa couplings which generate the CP asymmetries in the visible and dark matter sectors.
View original:
http://arxiv.org/abs/1206.0009
No comments:
Post a Comment