Dirac dark matter, neutrino masses, and dark baryogenesis

被引:0
|
作者
Restrepo, Diego [1 ,2 ]
Rivera, Andres [1 ]
Tangarife, Walter [3 ]
机构
[1] Univ Antioquia, Inst Fis, Calle 70 52-21, Medellin, Colombia
[2] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083859 Campinas, SP, Brazil
[3] Loyola Univ Chicago, Dept Phys, 1032 W Sheridan Rd, Chicago, IL 60660 USA
基金
巴西圣保罗研究基金会; 美国国家科学基金会;
关键词
MODEL; PROGRAM; SPHENO;
D O I
10.1103/PhysRevD.106.055021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a gauged baryon number model as an example of models where all new fermions required to cancel out the anomalies help to solve phenomenological problems of the standard model (SM). Dark fermion doublets, along with the isosinglet charged fermions, in conjunction with a set of SM-singlet fermions, participate in the generation of small neutrino masses through the Dirac-dark Zee mechanism. The other SM-singlets explain the dark matter in the Universe, while their coupling to an inert singlet scalar is the source of the CP violation. In the presence of a strong first-order electroweak phase transition, this "dark" CP violation allows for a successful electroweak baryogenesis mechanism.
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页数:12
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