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dc.contributor.authorDraper, Patrick
dc.contributor.authorMeade, Patrick
dc.contributor.authorReece, Matthew
dc.contributor.authorShih, David
dc.date.accessioned2019-09-26T15:01:30Z
dc.date.issued2012
dc.identifier.citationDraper, Patrick, Patrick Meade, Matthew Reece, and David Shih. 2012. “Implications of a 125 GeV Higgs Boson for the MSSM and Low-Scale Supersymmetry Breaking.” Physical Review D 85 (9). https://doi.org/10.1103/physrevd.85.095007.
dc.identifier.issn1550-2368
dc.identifier.issn1550-7998
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41412192*
dc.description.abstractRecently, the ATLAS and CMS collaborations have announced exciting hints for a standard model-like Higgs boson at a mass of approximate to 125 GeV. In this paper, we explore the potential consequences for the MSSM and low-scale SUSY-breaking. As is well-known, a 125 GeV Higgs implies either extremely heavy stops (>= 10 TeV), or near-maximal stop mixing. We review and quantify these statements, and investigate the implications for models of low-scale SUSY-breaking such as gauge mediation where the A-terms are small at the messenger scale. For such models, we find that either a gaugino must be superheavy or the NLSP is long-lived. Furthermore, stops will be tachyonic at high scales. These are very strong restrictions on the mediation of supersymmetry breaking in the MSSM, and suggest that if the Higgs truly is at 125 GeV, viable models of gauge-mediated supersymmetry breaking are reduced to small corners of parameter space or must incorporate new Higgs-sector physics.
dc.language.isoen_US
dc.publisherAmerican Physical Society
dash.licenseOAP
dc.titleImplications of a 125 GeV Higgs boson for the MSSM and low-scale supersymmetry breaking
dc.typeJournal Article
dc.description.versionAccepted Manuscript
dc.relation.journalPhysical Review D - Particles, Fields, Gravitation, and Cosmology
dash.depositing.authorReece, Matthew::21b33fac130fc9a9084fcaa1a6873bd6::600
dc.date.available2019-09-26T15:01:30Z
dash.workflow.comments1Science Serial ID 77274
dc.identifier.doi10.1103/PhysRevD.85.095007
dash.source.volume85;9


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