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Kinetically Modified Non-Minimal Higgs Inflation in Supergravity

High Energy Physics - Phenomenology 2016-01-22 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

We consider models of chaotic inflation driven by the real parts of a conjugate pair of Higgs superfields involved in the spontaneous breaking of a grand unification symmetry at a scale assuming its supersymmetric value. We combine a superpotential, which is uniquely determined by applying a continuous R symmetry, with a class of logarithmic or semi-logarithmic Kahler potentials which exhibit a prominent shift-symmetry with a tiny violation, whose strengths are quantified by c- and c+ respectively. The inflationary observables provide an excellent match to the recent BICEP2/Keck Array and Planck results setting 3.5x10^-3<=r+-=c+/c-<=1/N where N=3 or 2 is the prefactor of the logarithm. Inflation can be attained for subplanckian inflaton values with the corresponding effective theories retaining the perturbative unitarity up to the Planck scale.

Keywords

Cite

@article{arxiv.1511.01456,
  title  = {Kinetically Modified Non-Minimal Higgs Inflation in Supergravity},
  author = {C. Pallis},
  journal= {arXiv preprint arXiv:1511.01456},
  year   = {2016}
}

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R2 v1 2026-06-22T11:37:43.083Z