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Phenomenology of the Zee model for Dirac neutrinos and general neutrino interactions

机译:Dirac Neutrinos Zee模型的现象学和一般中氨基相互作用

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The Zee model for Dirac neutrinos is one of the simplest models featuring one-loop Dirac neutrino masses. The interactions between the new scalars (two singly charged fields) and neutrinos induce general neutrino interactions (GNI) which, as a generalization of the nonstandard neutrino interactions, constitute an additional tool to probe models beyond the Standard Model like this. In this work, we consider a U ( 1 ) B ? L gauge symmetry as being responsible for the Diracness of the neutrinos and the radiative character of the neutrino masses. We determine the viable parameter space consistent with neutrino oscillation data, leptonic rare decays, and collider constraints, and establish the most relevant experimental prospects regarding lepton flavor violation searches and GNI in future solar neutrino experiments.
机译:Dirac Neutrinos的Zee模型是一个最简单的模型之一,具有单环Dirac Neutrino Masses。 新的标渣(两个单电压)和中微子之间的相互作用诱导一般的中性细胞相互作用(GNI),其作为非标准中基相互作用的概括,构成了探测器模型之外的额外工具,如此。 在这项工作中,我们考虑一个U(1)B? L仪表对称性是负责中微子的Diraciss和中微子质量的辐射特征。 我们确定与中微子振荡数据一致的可行参数空间,轻型稀有衰减和碰撞者约束,并在未来的太阳中子实验中确定Lepton风味搜索和GNI的最相关的实验前景。

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