Pure Leptonic Gauge Symmetry, Neutrino Masses and Dark Matter
Pure Leptonic Gauge Symmetry, Neutrino Masses and Dark Matter
A possible extension of the Standard Model to include lepton number as local gauge symmetry is investigated. In such a model, anomalies are canceled by two extra fermions doublet. After leptonic gauge symmetry spontaneously broken, three active neutrinos may acquire non-zero Majorana masses through the modified Type-II seesaw mechanism. Constraints on the model from electro-weak precision measurements are studied. Due to the $Z_2$ discrete flavor symmetry, right-handed Majorana neutrinos can serve as cold dark matter candidate of the Universe. Constraint from dark matter relic abundance is calculated.
Wei Chao
10.1016/j.physletb.2010.10.056
物理学
Wei Chao.Pure Leptonic Gauge Symmetry, Neutrino Masses and Dark Matter[EB/OL].(2010-05-06)[2025-05-15].https://arxiv.org/abs/1005.1024.点此复制
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