F-Term Hybrid Inflation with T-Model Kähler Geometry and Beyond

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Autori principali: Ahmed, Waqas, Pallis, Constantinos, Rehman, Mansoor Ur
Natura: Preprint
Pubblicazione: 2026
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author Ahmed, Waqas
Pallis, Constantinos
Rehman, Mansoor Ur
author_facet Ahmed, Waqas
Pallis, Constantinos
Rehman, Mansoor Ur
contents We analyze F-term hybrid inflation (FHI) within various grand unified theories (GUTs) in the presence of a Kähler potential for the inflaton field which parameterizes the Kähler manifolds $SU(1,1)/U(1)$ or $SU(2)/U(1)$. We take into account supergravity, radiative, and soft supersymmetry-breaking corrections to the tree-level potential and find that viable FHI can be realized without extrema along the inflationary trajectory for a broad region of the parameter space. For selected superpotential parameters the models' predictions are largely influenced by the curvature of the internal space and the magnitude of the tadpole parameter which are constrained so as to achieve compatibility with the current ACT and SPT data. We also discuss the formation of cosmic strings and their associated gravitational wave signals, potentially detectable by current and upcoming experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2605_08931
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle F-Term Hybrid Inflation with T-Model Kähler Geometry and Beyond
Ahmed, Waqas
Pallis, Constantinos
Rehman, Mansoor Ur
High Energy Physics - Phenomenology
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We analyze F-term hybrid inflation (FHI) within various grand unified theories (GUTs) in the presence of a Kähler potential for the inflaton field which parameterizes the Kähler manifolds $SU(1,1)/U(1)$ or $SU(2)/U(1)$. We take into account supergravity, radiative, and soft supersymmetry-breaking corrections to the tree-level potential and find that viable FHI can be realized without extrema along the inflationary trajectory for a broad region of the parameter space. For selected superpotential parameters the models' predictions are largely influenced by the curvature of the internal space and the magnitude of the tadpole parameter which are constrained so as to achieve compatibility with the current ACT and SPT data. We also discuss the formation of cosmic strings and their associated gravitational wave signals, potentially detectable by current and upcoming experiments.
title F-Term Hybrid Inflation with T-Model Kähler Geometry and Beyond
topic High Energy Physics - Phenomenology
General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2605.08931