作者: J.G. Ferreira , C.A. de S. Pires , J.G. Rodrigues , P.S. Rodrigues da Silva
DOI: 10.1016/J.PHYSLETB.2017.05.034
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摘要: Abstract The Peccei–Quinn symmetry is an intrinsic global of the 3-3-1 gauge models. Its spontaneous breaking mechanism engendering invisible KSVZ-like axion links models with new physics at ∼ 10 GeV scale. that results from this interesting candidate for dark matter universe, while its real partner may drive inflation if radiative corrections are taken into account. This obtained by connecting type I seesaw symmetry. In end day we have a scenario providing common answer to strong-CP problem, inflation, and neutrino mass.