Dark matter assisted lepton anomalous magnetic moments and neutrino masses

被引:57
|
作者
Jana, Sudip [1 ]
Vishnu, P. K. [2 ]
Rodejohann, Werner [1 ]
Saad, Shaikh [2 ]
机构
[1] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
[2] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA
关键词
MUON; G-2; MODEL;
D O I
10.1103/PhysRevD.102.075003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a framework that addresses the origin of neutrino mass, explains the observed discrepancies in the electron and the muon anomalous magnetic moments (AMMs) data, and incorporates the dark matter (DM) relic abundance. Both the neutrino mass and the lepton AMMs are generated at one-loop level mediated by a common set of beyond the Standard Model (SM) states. In this class of models, the SM is extended with vectorlike charged fermion and scalar multiplets, all odd under an imposed Z(2) symmetry, which stabilizes the fermionic or scalar DM candidate residing in one of them. Two scalar multiplets appear in the AMM loops, thus allowing for different signs of their contributions, in agreement with the observed discrepancies which are of opposite sign for electron and muon. The vectorlike fermions give rise to large new physics contributions to the lepton AMMs via chirally enhanced terms that are proportional to their mass. To demonstrate the viability of this framework, we perform a detailed study of a particular model for which a fit to the neutrino masses and mixing together with lepton AMMs are provided. Furthermore, DM phenomenology and collider signatures are explored.
引用
收藏
页数:16
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