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
相关论文
共 50 条
  • [21] Dark matter in the supersymmetric radiative seesaw model with an anomalous U(1) symmetry
    Suematsu, Daijiro
    Toma, Takashi
    NUCLEAR PHYSICS B, 2011, 847 (03) : 567 - 589
  • [22] (sub)GeV dark matter in the U(1)X Higgs portal model
    Amiri, Amir
    Saez, Bastian Diaz
    Ghorbani, Karim
    PHYSICS LETTERS B, 2023, 844
  • [23] A model of the matter-antimatter asymmetry and cold dark matter with U(1)B-L ⊗ U(1)D
    Yang, Wei-Min
    PHYSICS LETTERS B, 2016, 762 : 138 - 144
  • [24] Indirect detection of secluded supersymmetric dark matter
    Barnes, Patrick
    Johnson, Zachary
    Pierce, Aaron
    Shakya, Bibhushan
    PHYSICAL REVIEW D, 2022, 105 (03)
  • [25] Secluded dark matter coupled to a hidden CFT
    Benedict von Harling
    Kristian L. McDonald
    Journal of High Energy Physics, 2012
  • [26] Theoretical bounds on dark Higgs mass in a self-interacting dark matter model with U(1)'
    Li, Song
    Yang, Jin Min
    Zhang, Mengchao
    Zhu, Rui
    PHYSICAL REVIEW D, 2025, 111 (03)
  • [27] Secluded dark matter coupled to a hidden CFT
    von Harling, Benedict
    McDonald, Kristian L.
    JOURNAL OF HIGH ENERGY PHYSICS, 2012, (08):
  • [28] Radiative linear seesaw model, dark matter, and U(1)B-L
    Wang, Weijian
    Han, Zhi-Long
    PHYSICAL REVIEW D, 2015, 92 (09)
  • [29] Right-handed neutrino dark matter in a U(1) extension of the Standard Model
    Cox, Peter
    Han, Chengcheng
    Yanagida, Tsutomu T.
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2018, (01):
  • [30] Hidden gauged U(1) model: Unifying scotogenic neutrino and flavor dark matter
    Yu, Jiang-Hao
    PHYSICAL REVIEW D, 2016, 93 (11)