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Dirac Leptogenesis with a Non-anomalous U(1)^(prime) Family Symmetry

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arxiv 1111.5018 v2 pith:DF72HDF7 submitted 2011-11-21 hep-ph astro-ph.CO

Dirac Leptogenesis with a Non-anomalous U(1)^(prime) Family Symmetry

classification hep-ph astro-ph.CO
keywords diracleptogenesisfermionsmodelfamilymassesneutrinosnon-anomalous
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We propose a model for Dirac leptogenesis based on a non-anomalous $U(1)^{\prime}$ gauged family symmetry. The anomaly cancellation conditions are satisfied with no new chiral fermions other than the three right-handed neutrinos, giving rise to stringent constraints among the charges. Realistic masses and mixing angles are obtained for all fermions. The model predicts neutrinos of the Dirac type with naturally suppressed masses. Dirac leptogenesis is achieved through the decay of the flavon fields. The cascade decays of the vector-like heavy fermions in the Froggatt-Nielsen mechanism play a crucial role in the separation of the primodial lepton numbers. We find that a large region of parameter space of the model gives rise to a sufficient cosmological baryon number asymmetry through Dirac leptogenesis.

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