Model characterization and dark matter in the secluded U(1)' model

被引:4
|
作者
Hicyilmaz, Yasar [1 ,2 ]
Selbuz, Levent [3 ]
Solmaz, Levent [1 ]
Un, Cem Salih [4 ,5 ,6 ]
机构
[1] Balikesir Univ, Dept Phys, TR-10145 Balikesir, Turkey
[2] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
[3] Ankara Univ, Dept Engn Phys, TR-06100 Ankara, Turkey
[4] Bursa Uludag Univ, Dept Phys, TR-16059 Bursa, Turkey
[5] Univ Huelva, Dept Ciencias Integradas, Campus Carmen, Huelva 21071, Spain
[6] Univ Huelva, Ctr Estudios Avanzados Fis Matemat & Comp, Campus Carmen, Huelva 21071, Spain
关键词
SYMMETRY-BREAKING; BOSON MASS; GAUGE; UNIFICATION; DYNAMICS; SPHENO; FLAVOR; E6;
D O I
10.1103/PhysRevD.105.055029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a class of U(1)'-extended minimal supersymmetric extension of the Standard Model (MSSM) in which the U(1)' symmetry is broken by vacuum expectation values of four MSSM singlet fields. While one MSSM singlet field interacts with the MSSM Higgs fields, three of them interact only with each other in forming a secluded sector. Assigning universal U(1)' charges for three families, the anomaly cancellation condition requires exotic fields which are assumed to be heavy and decoupled. We discuss a variety of U(1)' charge assignments and anomaly cancellation, Z'/Z hierarchy, neutralinos, charginos and the Higgs sector. We find that the typical spectra involve two CP-odd Higgs bosons lighter than about 200 GeV and 600 GeV respectively, which are mostly formed by the MSSM singlet fields. If the relic density of dark matter is saturated only by a neutralino, compatible solutions predict LSP neutralinos formed by the MSSM singlet fields in the mass scales below about 600 GeV, while it is possible to realize MSSM neutralino LSP above these mass scales. One can classify the implications in three scenarios. Scenario I involves NLSP charginos, while Scenario II involves charginos which do not participate coannihilation processes with the LSP neutralino. These two scenarios predict MSSM singlet LSP neutralinos, while Scenario I leads to larger scattering cross sections of dark matter. Scenario III has the solutions in which the MSSM neutralinos are considerably involved in LSP decomposition which yields very large scattering cross section excluded by the direct detection experiments.
引用
收藏
页数:20
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