English

F-Term Hybrid Inflation and SUSY Breaking

High Energy Physics - Phenomenology 2025-04-04 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

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.

Keywords

Cite

@article{arxiv.2504.02121,
  title  = {F-Term Hybrid Inflation and SUSY Breaking},
  author = {C. Pallis},
  journal= {arXiv preprint arXiv:2504.02121},
  year   = {2025}
}

Comments

Prepared for the Proceedings of the Workshop on the Standard Model and Beyond, Corfu Summer Institute 2024

R2 v1 2026-06-28T22:44:31.983Z