6,945 research outputs found

    The naturalness in the BLMSSM and B-LSSM

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    In order to interpret the Higgs mass and its decays more naturally, we hope to intrude the BLMSSM and B-LSSM. In the both models, the right-handed neutrino superfields are introduced to better explain the neutrino mass problems. In addition, there are other superfields considered to make these models more natural than MSSM. In this paper, the method of χ2\chi^2 analyses will be adopted in the BLMSSM and B-LSSM to calculate the Higgs mass, Higgs decays and muon g−2g-2. With the fine-tuning in the region 0.67%−2.5%0.67\%-2.5\% and 0.67%−5%0.67\%-5\%, we can obtain the reasonable theoretical values that are in accordance with the experimental results respectively in the BLMSSM and B-LSSM. Meanwhile, the best-fitted benchmark points in the BLMSSM and B-LSSM will be acquired at minimal (χminBL)2=2.34736(\chi^{BL}_{min})^2 = 2.34736 and (χminB−L)2=2.47754(\chi^{B-L}_{min})^2 = 2.47754, respectively

    The extended BLMSSM with a 125 GeV Higgs boson and dark matter

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    To extend the BLMSSM, we not only add exotic Higgs superfields (ΦNL,φNL)(\Phi_{NL},\varphi_{NL}) to make the exotic lepton heavy, but also introduce the superfields(YY,Y′Y^\prime) having couplings with lepton and exotic lepton at tree level. The obtained model is called as EBLMSSM, which has difference from BLMSSM especially for the exotic slepton(lepton) and exotic sneutrino(neutrino). We deduce the mass matrices and the needed couplings in this model. To confine the parameter space, the Higgs boson mass mh0m_{h^0} and the processes h0→γγh^0\rightarrow \gamma\gamma, h0→VV,V=(Z,W)h^0\rightarrow VV, V=(Z,W) are studied in the EBLMSSM. With the assumed parameter space, we obtain reasonable numerical results according to data on Higgs from ATLAS and CMS. As a cold dark mater candidate, the relic density for the lightest mass eigenstate of YY and Y′Y' mixing is also studied
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