Radiative Symmetry Breaking and Higgs Mass Bound in the NMSSM
Radiative Symmetry Breaking and Higgs Mass Bound in the NMSSM
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NMSSM 中的辐射对称破缺和希格斯质量束缚
DOI:
10.1143/ptp.104.827
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发表时间:
2000
期刊:
影响因子:
--
通讯作者:
D. Suematsu
中科院分区:
文献类型:
--
作者:
Y. Daikoku;D. Suematsu
We study the mass upper bound of the lightest neutral Higgs scalar in the next to minimal supersymmetric standard model (NMSSM) using RGE analysis. We require electroweak radiative symmetry breaking in order to restrict the parameter space. As a result, the mass upper bound mh0 is severely constrained compared with that calculated without imposing this condition. We point out some features of mh0 related to the initial value of ht and discuss why models with more extra matter fields 5 + ¯ of SU(5) yield larger maximum value of mh0 . The existence of a rather light CP-even neutral Higgs scalar is a common feature of supersymmetric extensions of the standard model. 1),2) Experimental confirmation of this predicted property would provide important evidence for the validity of these models. It would be useful to compare the mass upper bounds for this particle in these models to judge their consistency. The next to minimal supersymmetric standard model (NMSSM) is the simplest extension of the minimal supersymmetric standard model (MSSM). 3) In this model, a singlet chiral supermultiplet S is introduced, and the µ term in the MSSM is replaced by the Yukawa coupling λSH1H2, where H1 and H2 are the usual doublet Higgs chiral superfields. The superpotential of the Higgs sector in this model is expressed as