A SM-like Higgs near 125 GeV in low energy SUSY: a comparative study for MSSM and NMSSM
A bstract Motivated by the recent LHC hints of a Higgs boson around 125 GeV, we assume a SM-like Higgs with the mass 123-127 GeV and study its implication in low energy SUSY by comparing the MSSM and NMSSM. We consider various experimental constraints at 2 σ level (including the muon g − 2 and the d...
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Veröffentlicht in: | The journal of high energy physics 2012-03, Vol.2012 (3) |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | A
bstract
Motivated by the recent LHC hints of a Higgs boson around 125 GeV, we assume a SM-like Higgs with the mass 123-127 GeV and study its implication in low energy SUSY by comparing the MSSM and NMSSM. We consider various experimental constraints at 2
σ
level (including the muon
g
− 2 and the dark matter relic density) and perform a comprehensive scan over the parameter space of each model. Then in the parameter space which is allowed by current experimental constraints and also predicts a SM-like Higgs in 123-127 GeV, we examine the properties of the sensitive parameters (like the top squark mass and the trilinear coupling
A
t
) and calculate the rates of the di-photon signal and the
V V
*
(
V
=
W, Z
) signals at the LHC. Our typical findings are: (i) In the MSSM the top squark and
A
t
must be large and thus incur some fine-tuning, which can be much ameliorated in the NMSSM; (ii) In the MSSM a light stau is needed to enhance the di- photon rate of the SM-like Higgs to exceed its SM prediction, while in the NMSSM the di-photon rate can be readily enhanced in several ways; (iii) In the MSSM the signal rates of
pp
→
h
→
V V
*
at the LHC are never enhanced compared with their SM predictions, while in the NMSSM they may get enhanced significantly; (iv) A large part of the parameter space so far survived will be soon covered by the expected XENON100(2012) sensitivity (especially for the NMSSM). |
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ISSN: | 1029-8479 |
DOI: | 10.1007/JHEP03(2012)086 |