Triplet Extended MSSM : Fine Tuning vs Perturbativity & Experiment

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dc.contributor.author Bandyopadhyay, Priyotosh
dc.contributor.author Di Chiara, Stefano
dc.contributor.author Huitu, Katri
dc.contributor.author Keceli, Asli Sabanci
dc.date.accessioned 2017-09-01T05:52:01Z
dc.date.available 2017-09-01T05:52:01Z
dc.date.issued 2016
dc.identifier.citation Bandyopadhyay , P , Di Chiara , S , Huitu , K & Keceli , A S 2016 , ' Triplet Extended MSSM : Fine Tuning vs Perturbativity & Experiment ' , Nuclear and particle physics proceedings , vol. 273 , pp. 595-601 . https://doi.org/10.1016/j.nuclphysbps.2015.09.089
dc.identifier.other PURE: 78951978
dc.identifier.other PURE UUID: 0fb6e2cf-5f9f-46d4-9e5e-9fe36bc1ce0a
dc.identifier.other WOS: 000390295200088
dc.identifier.other Scopus: 84973097508
dc.identifier.other ORCID: /0000-0002-7754-9320/work/29936866
dc.identifier.uri http://hdl.handle.net/10138/218278
dc.description Volume: 273
dc.description.abstract In this study we investigate the phenomenological viability of the Y = 0 Triplet Extended Supersymmetric Standard Model (TESSM) by comparing its predictions with the current Higgs data from ATLAS, CMS, and Tevatron, as well as the measured value of the B-S -> X-S gamma branching ratio. We scan numerically the parameter space for data points generating the measured particle mass spectrum and also satisfying current direct search constraints on new particles. We require all the couplings to be perturbative up to the scale A(UV) = 10(4) TeV, by running them with newly calculated two loop beta functions, and find that TESSM retains perturbativity as long as A, the triplet coupling to the two Higgs doublets, is smaller than 1.34 in absolute value. For vertical bar lambda vertical bar greater than or similar to 0.8 we show that the fine-tuning associated to each viable data point can be greatly reduced as compared to values attainable in MSSM. Finally, we perform a fit by taking into account 58 Higgs physics observables along with Br(B-s -> X-s gamma), for which we calculate the NLO prediction within TESSM. We find that, although naturality prefers a large vertical bar lambda vertical bar, the experimental data disfavors it compared to the small vertical bar lambda vertical bar region, because of the low energy observable Br(B-s -> X-s gamma). en
dc.format.extent 7
dc.language.iso eng
dc.relation.ispartof Nuclear and particle physics proceedings
dc.rights cc_by
dc.rights.uri info:eu-repo/semantics/openAccess
dc.subject Higgs
dc.subject Triplet Higgs
dc.subject Supersymmetry
dc.subject LEADING QCD CORRECTIONS
dc.subject STANDARD MODEL
dc.subject MASSES
dc.subject 114 Physical sciences
dc.title Triplet Extended MSSM : Fine Tuning vs Perturbativity & Experiment en
dc.type Conference article
dc.contributor.organization Department of Physics
dc.contributor.organization Helsinki Institute of Physics
dc.description.reviewstatus Peer reviewed
dc.relation.doi https://doi.org/10.1016/j.nuclphysbps.2015.09.089
dc.relation.issn 2405-6014
dc.rights.accesslevel openAccess
dc.type.version publishedVersion

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