(g-2)e,μ and strongly interacting dark matter with collider implications

被引:12
|
作者
Biswas, Anirban [1 ,2 ]
Khan, Sarif [3 ]
机构
[1] Sogang Univ, Dept Phys, Seoul 121742, South Korea
[2] Sogang Univ, Ctr Quantum Spacetime, Seoul 121742, South Korea
[3] Georg August Univ Gottingen, Inst Theoret Phys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany
基金
新加坡国家研究基金会;
关键词
Cosmology of Theories BSM; Early Universe Particle Physics; Particle Nature of Dark Matter; Specific BSM Phenomenology; MU-L-TAU; ANOMALOUS MAGNETIC-MOMENT; GAUGED L-MU; NEUTRINO MASS; SYMMETRY;
D O I
10.1007/JHEP07(2022)037
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
The quest for new physics beyond the Standard Model is boosted by the recently observed deviation in the anomalous magnetic moments of muon and electron from their respective theoretical prediction. In the present work, we have proposed a suitable extension of the minimal L-mu - L-tau model to address these two experimental results as the minimal model is unable to provide any realistic solution. In our model, a new Yukawa interaction involving first generation of leptons, a singlet vector like fermion (chi(+/-)) and a scalar (either an SU(2)(L) doublet Phi(2)' or a complex singlet Phi(4)') provides the additional one loop contribution to a(e) only on top of the usual contribution coming from the L-mu- L-tau gauge boson (Z(mu tau)) to both electron and muon. The judicious choice of L-mu - L-tau charges to these new fields results in a strongly interacting scalar dark matter in O (MeV) range after taking into account the bounds from relic density, unitarity and self interaction. The freeze-out dynamics of dark matter is greatly influenced by 3 -> 2 scatterings while the kinetic equilibrium with the SM bath is ensured by 2 -> 2 scatterings with neutrinos where Z(mu tau) plays a pivotal role. The detection of dark matter is possible directly through scatterings with nuclei mediated by the SM Z bosons. Moreover, our proposed model can also be tested in the upcoming e(+)e(-) colliders by searching opposite sign di-electron and missing energy signal i.e. at the final state.
引用
收藏
页数:44
相关论文
共 50 条
  • [1] (g − 2)e, μ and strongly interacting dark matter with collider implications
    Anirban Biswas
    Sarif Khan
    Journal of High Energy Physics, 2022
  • [2] (g-2)μ and stau coannihilation: dark matter and collider analysis
    Chakraborti, Manimala
    Heinemeyer, Sven
    Saha, Ipsita
    EUROPEAN PHYSICAL JOURNAL C, 2024, 84 (02):
  • [3] Connection of g-2μ, electroweak, dark matter, and collider constraints on 331 models
    Kelso, Chris
    Long, H. N.
    Martinez, R.
    Queiroz, Farinaldo S.
    PHYSICAL REVIEW D, 2014, 90 (11):
  • [4] (g-2)μ and SUSY dark matter: direct detection and collider search complementarity
    Chakraborti, Manimala
    Heinemeyer, Sven
    Saha, Ipsita
    Schappacher, Christian
    EUROPEAN PHYSICAL JOURNAL C, 2022, 82 (05):
  • [5] 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):
  • [6] A 2HDM for the g-2 and dark matter
    Arcadi, Giorgio
    de Jesus, Alvaro S.
    de Melo, Tessio B.
    Queiroz, Farinaldo S.
    Villamizar, Yoxara S.
    NUCLEAR PHYSICS B, 2022, 982
  • [7] Dark Matter and (g-2)μ,e in radiative Dirac neutrino mass models
    Chowdhury, Talal Ahmed
    Ehsanuzzaman, Md.
    Saad, Shaikh
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2022, (08):
  • [8] Collider probe of heavy additional Higgs bosons solving the muon g-2 and dark matter problems
    Blanke, Monika
    Iguro, Syuhei
    PHYSICAL REVIEW D, 2023, 107 (09)
  • [9] A SEARCH FOR STRONGLY INTERACTING DARK MATTER
    RICH, J
    ROCCHIA, R
    SPIRO, M
    PHYSICS LETTERS B, 1987, 194 (01) : 173 - 176
  • [10] Composite strongly interacting dark matter
    Cline, James M.
    Liu, Zuowei
    Moore, Guy D.
    Xue, Wei
    PHYSICAL REVIEW D, 2014, 90 (01)