Improved (g-2)μ measurement and singlino dark matter in μ-term extended Z3-NMSSM

被引:46
|
作者
Cao, Junjie [1 ]
Lian, Jingwei [1 ]
Pan, Yusi [1 ]
Zhang, Di [1 ]
Zhu, Pengxuan [1 ]
机构
[1] Henan Normal Univ, Dept Phys, Xinxiang 453007, Henan, Peoples R China
关键词
Supersymmetry Phenomenology; ANOMALOUS MAGNETIC-MOMENT; SUPERSYMMETRIC 2-LOOP CORRECTIONS; RELIC DENSITY; HIGGS-BOSON; MODEL; PROGRAM; MSSM; PHYSICS; TOOL; SUPERGRAVITY;
D O I
10.1007/JHEP09(2021)175
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Very recently, a Fermilab report of muon g - 2 showed a 4.2 sigma discrepancy between it and the standard model (SM) prediction. Motivated by this inspiring result and the increasing tension in supersymmetric interpretation of the anomalous magnetic moment, it is argued that in the general next-to-minimal supersymmetric standard model (GNMSSM), a singlino-dominated neutralino can act as a feasible dark matter (DM) candidate in explaining the discrepancy naturally. In this case, the singlino-dominated DM and singlet-dominated Higgs bosons can form a secluded DM sector with (chi) over tilde (0)(1)(chi) over tilde (0)(1) -> h(s)A(s) responsible for the measured DM relic abundance when m((chi) over tilde 10) greater than or similar to 150 GeV and the Yukawa coupling kappa is around 0.2. This sector communicates with the SM sector by weak singlet-doublet Higgs mixing, so the scatterings of the singlino-dominated DM with nucleons are suppressed. Furthermore, due to the singlet nature of the DM and the complex mass hierarchy, sparticle decay chains in the GNMSSM are lengthened in comparison with the prediction of the minimal supersymmetric standard model. These characteristics lead to sparticle detection at the Large Hadron Collider (LHC) being rather tricky. This study surveys a specific scenario of the GNMSSM, which extends the Z(3)-NMSSM by adding an explicit mu-term, to reveal the features. It indicates that the theory can readily explain the discrepancy of the muon anomalous magnetic moment without conflicting with the experimental results in DM and Higgs physics, and the LHC searches for sparticles.
引用
收藏
页数:36
相关论文
共 50 条
  • [1] Improved (g − 2)μ measurement and singlino dark matter in μ-term extended ℤ3-NMSSM
    Junjie Cao
    Jingwei Lian
    Yusi Pan
    Di Zhang
    Pengxuan Zhu
    Journal of High Energy Physics, 2021
  • [2] Impact of LHC probes of SUSY and recent measurement of (g-2)μ on Z3-NMSSM
    Cao, Junjie
    Li, Fei
    Lian, Jingwei
    Pan, Yusi
    Zhang, Di
    SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2022, 65 (09)
  • [3] Singlino-dominated dark matter in Z3-symmetric NMSSM
    Zhou, Haijing
    Cao, Junjie
    Lian, Jingwei
    Zhang, Di
    PHYSICAL REVIEW D, 2021, 104 (01)
  • [4] Revisiting singlino dark matter of the natural Z3-symmetric NMSSM in the light of LHC
    Abdallah, Waleed
    Chatterjee, Arindam
    Datta, AseshKrishna
    JOURNAL OF HIGH ENERGY PHYSICS, 2019, 2019 (09)
  • [5] W-boson mass, dark matter and muon (g-2) in the μNMSSM
    Heng, Zhaoxia
    Li, Xingjuan
    Shang, Liangliang
    INTERNATIONAL JOURNAL OF MODERN PHYSICS A, 2023,
  • [6] Improved (g-2)μ measurements and wino/higgsino dark matter
    Chakraborti, Manimala
    Heinemeyer, Sven
    Saha, Ipsita
    EUROPEAN PHYSICAL JOURNAL C, 2021, 81 (12):
  • [7] Revisiting singlino dark matter of the natural Z3-symmetric NMSSM in the light of LHC
    Waleed Abdallah
    Arindam Chatterjee
    AseshKrishna Datta
    Journal of High Energy Physics, 2019
  • [8] Expectations for the muon g-2 in simplified models with dark matter
    Kowalska, Kamila
    Sessolo, Enrico Maria
    JOURNAL OF HIGH ENERGY PHYSICS, 2017, (09):
  • [9] SUSY Dark Matter Direct Detection Prospects Based on (g-2)μ
    Chakraborti, Manimala
    Heinemeyer, Sven
    Saha, Ipsita
    MOSCOW UNIVERSITY PHYSICS BULLETIN, 2022, 77 (02) : 116 - 119
  • [10] Implications of Sgr A∗ on the γ-rays searches of Bino dark matter with (g-2)μ
    Chattopadhyay, Utpal
    Das, Debottam
    Poddar, Sujoy
    Puri, Rahul
    Saha, Abhijit Kumar
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2025, (120):