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Solving The Muon g-2 Anomaly With Natural NMSSM From Generalized Deflected AMSB

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arxiv 1704.05079 v2 pith:44BZG26N submitted 2017-04-17 hep-ph

classification hep-ph
keywords anomalymuonnaturalnmssmamsbdeflectedinteractionsmessenger-matter
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We propose to realize (natural) NMSSM spectrum from deflected AMSB with new messenger-matter interactions. With additional messenger-matter interactions involving ${\bf 10}\oplus{\bf \overline{10}}$ representation messengers, the muon g-2 anomaly can be solved at $2\sigma$ (or $3\sigma$) level with the corresponding gluino mass range $2.8~{\rm TeV}<m_{\tilde{g}}<5.4~ {\rm TeV}$ (or $2.6 ~{\rm TeV}<m_{\tilde{g}}<7.3~ {\rm TeV}$). Besides, our scenario is fairly natural within which the involved fine tuning can be as low as 47. So, in the framework of AMSB-type scenarios, NMSSM can be advantageous in explaining the muon g-2 anomaly in compare with MSSM.

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  1. The LHC sensitivity to weak gauginos in light of the latest muon $g-2$ and dark matter results

    hep-ph 2025-05 conditional novelty 4.0 of 10

    In the MSSM, after muon g-2 and dark matter constraints, only bino-like LSPs with wino or slepton coannihilation survive, and a 27 TeV HE-LHC could probe most of the remaining mass range.

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