Electroweak supersymmetry in the NMSSM

被引:21
|
作者
Cheng, Taoli [1 ]
Li, Tianjun [1 ,2 ,3 ]
机构
[1] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
[2] Univ Elect Sci & Technol China, Sch Phys Elect, Chengdu 610054, Peoples R China
[3] Texas A&M Univ, George P & Cynthia W Mitchell Inst Fundamental Ph, College Stn, TX 77843 USA
关键词
HIGGS;
D O I
10.1103/PhysRevD.88.015031
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
To explain all the available experimental results, we have proposed the electroweak supersymmetry (EWSUSY) previously, where the squarks and/or gluino are heavy around a few TeVs while the sleptons, sneutrinos, bino, winos, and/or Higgsinos are light within 1 TeV. In the next to minimal supersymmetric Standard Model, we perform the systematic chi(2) analyses on parameter space scan for three EWSUSY scenarios: (I) R-parity conservation and one dark matter candidate, (II) R-parity conservation and multicomponent dark matter, (III) R-parity violation. We obtain the minimal chi(2)/(degree of freedom) of 10.2/15, 9.6/14, and 9.2/14 respectively for scenarios I, II, and III. Considering the constraints from the LHC neutralino/chargino and slepton searches, we find that the majority of viable parameter space preferred by the muon anomalous magnetic moment has been excluded except for the parameter space with moderate to large tan beta(greater than or similar to 8). Especially, the most favorable parameter space has relatively large tan beta, moderate lambda, small mu(eff), heavy squarks/gluino, and the second lightest CP-even neutral Higgs boson with mass around 125 GeV. In addition, if the left-handed smuon is nearly degenerate with or heavier than wino, there is no definite bound on wino mass. Otherwise, the wino with mass up to similar to 450 GeV has been excluded. Furthermore, we present several benchmark points for scenarios I and II, and briefly discuss the prospects of the EWSUSY searches at the 14 TeV LHC and ILC.
引用
收藏
页数:18
相关论文
共 50 条
  • [1] Electroweak baryogenesis in the nMSSM
    Konstandin, T.
    SUSY06: THE 14TH INTERNATIONAL CONFERENCE ON SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS, 2007, 903 : 689 - 692
  • [2] Supersymmetry beyond the NMSSM
    Staub, Florian
    Goodsell, Mark D.
    Malinsky, Michal
    Schmidt-Hoberg, Kai
    ADVANCES IN HIGH ENERGY PHYSICS, 2015, 2015
  • [3] Split NMSSM with electroweak baryogenesis
    Demidov, S. V.
    Gorbunov, D. S.
    Kirpichnikov, D. V.
    JOURNAL OF HIGH ENERGY PHYSICS, 2016, (11):
  • [4] Split NMSSM with electroweak baryogenesis
    S. V. Demidov
    D. S. Gorbunov
    D. V. Kirpichnikov
    Journal of High Energy Physics, 2016
  • [5] Electroweak supersymmetry around the electroweak scale
    Taoli Cheng
    Jinmian Li
    Tianjun Li
    Dimitri V. Nanopoulos
    Chunli Tong
    The European Physical Journal C, 2013, 73
  • [6] Electroweak phase transition and baryogenesis in the nMSSM
    Huber, Stephan J.
    Konstandin, Thomas
    Prokopec, Tomislav
    Schmidt, Michael G.
    NUCLEAR PHYSICS B, 2006, 757 (1-2) : 172 - 196
  • [7] Electroweak supersymmetry around the electroweak scale
    Cheng, Taoli
    Li, Jinmian
    Li, Tianjun
    Nanopoulos, Dimitri V.
    Tong, Chunli
    EUROPEAN PHYSICAL JOURNAL C, 2013, 73 (02): : 1 - 11
  • [8] Erratum to: Split NMSSM with electroweak baryogenesis
    S. V. Demidov
    D. S. Gorbunov
    D. V. Kirpichnikov
    Journal of High Energy Physics, 2017
  • [9] Supersymmetry at the electroweak scale
    Chankowski, PH
    Pokorski, S
    ACTA PHYSICA POLONICA B, 1996, 27 (08): : 1719 - 1737
  • [10] Supersymmetry at the electroweak scale
    Chankowski, PH
    Pokorski, S
    NUCLEAR PHYSICS B, 1997, : 43 - 54