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Hybrid Inflation with Quasi-canonical Supergravity

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arxiv hep-ph/9703443 v2 pith:ATUK3HY3 submitted 1997-03-27 hep-ph astro-ph

Hybrid Inflation with Quasi-canonical Supergravity

C. Panagiotakopoulos (Physics Division , School of Technology , University of Thessaloniki , Thessaloniki , Greece) This is my paper
classification hep-ph astro-ph
keywords hybridinflationinflationarymodelquasi-canonicalsupergravityadiabaticalong
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We construct a hybrid inflationary model associated with the superheavy scale of the minimal supersymmetric standard model which is based on the simplest superpotential for symmetry breaking and in which the inflaton potential along the inflationary trajectory is essentially provided by quasi-canonical supergravity. The resulting spectrum of adiabatic density perturbations is blue and the duration of inflation sufficient but rather limited.

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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...