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F-Term Hybrid Inflation and SUSY Breaking

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arxiv 2504.02121 v1 pith:EFK3WBOV submitted 2025-04-02 hep-ph astro-ph.COhep-th

F-Term Hybrid Inflation and SUSY Breaking

classification hep-ph astro-ph.COhep-th
keywords breakingf-termhybridinflationkaehlermasssupersymmetrysymmetry
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We consider F-term hybrid inflation and supersymmetry breaking in the context of a model which largely respects a global U(1) R symmetry. The Kaehler potential parameterizes the Kaehler manifold with an enhanced U(1)_Rx(SU(1,1)/U(1)) symmetry, where the scalar curvature of the second factor is determined by the achievement of a supersymmetry-breaking de Sitter vacuum without ugly tuning. The magnitude of the emergent soft tadpole term for the inflaton can be adjusted in the range (1.2-460) TeV -- increasing with the dimensionality of the representation of the waterfall fields -- so that the inflationary observables are in agreement with the observational requirements. The mass scale of the supersymmetric partners turns out to lie in the region (0.09-253) PeV which is compatible with high-scale supersymmetry and the results of LHC on the Higgs boson mass. The mu parameter can be generated by conveniently applying the Giudice-Masiero mechanism and assures the out-of-equilibrium decay of the R saxion at a low reheat temperature Trh<163 GeV.

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  1. F-Term Hybrid Inflation with T-Model K\"ahler Geometry and Beyond

    hep-ph 2026-05 unverdicted novelty 4.0

    F-term hybrid inflation with SU(1,1)/U(1) or SU(2)/U(1) Kähler geometry in GUTs can be realized without inflationary extrema for broad parameters, matching ACT/SPT data via curvature and tadpole adjustments while pred...