Constraining the 3-3-1 model with heavy neutral leptons using (g 2)μ and dark matter observables

被引:4
作者
Alvarez-Salazar, C. E. [1 ,2 ]
Peres, O. L. G. [2 ]
机构
[1] Univ Manuela Beltran, Lab Fis, Ave Circunvalar 60-00, Bogota 110231, DC, Colombia
[2] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083859 Campinas, SP, Brazil
基金
巴西圣保罗研究基金会;
关键词
GRAND UNIFICATION; SEARCHES; PHYSICS; WEAK;
D O I
10.1103/PhysRevD.103.035029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Models with gauge symmetry SU(3)(c) circle times SU(3)(L) circle times U(1)(N) have different candidates for dark matter, for example, a heavy neutral fermion interacting with standard model particles through different mediators, scalar and vector portals. At the same time, these portals can produce signals in the anomalous magnetic moment of the muon that violate the present bounds on this quantity. Combining the requirement to have a dark matter candidate in the SU(3)(c) circle times SU(3)(L) circle times U(1)(N) model with heavy neutral leptons and to explain the anomalous magnetic moment of the muon we set constraints on the highest symmetry breaking scale of the model. These bounds are competitive with the constraints from LHC and set a favored region that can also be tested in future direct detection experiments, such as the LUX-ZEPLIN (LZ) experiment.
引用
收藏
页数:15
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