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Main Authors: Christodoulidis, Perseas, Rosati, Robert, Sfakianakis, Evangelos I.
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2504.12406
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author Christodoulidis, Perseas
Rosati, Robert
Sfakianakis, Evangelos I.
author_facet Christodoulidis, Perseas
Rosati, Robert
Sfakianakis, Evangelos I.
contents Multi-field inflation can be inherently non-predictive, with the exception of models with strong attractors. In this work, we focus on models with multiple scalar fields that are non-minimally coupled to the space-time Ricci curvature scalar, motivated by the expectation of a rich particle spectrum at high energies. We show that in this family of models, the single- and multi-field predictions for CMB observables are identical, as long as there exists at least one non-minimal coupling with $ξ\gg 1$. We provide simple expressions for the Hubble scale, the number of $e$-folds, and the turn rate for systems with an arbitrary number of fields and explore the statistical properties for different priors.
format Preprint
id arxiv_https___arxiv_org_abs_2504_12406
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Robust non-minimal attractors in many-field inflation
Christodoulidis, Perseas
Rosati, Robert
Sfakianakis, Evangelos I.
Cosmology and Nongalactic Astrophysics
Multi-field inflation can be inherently non-predictive, with the exception of models with strong attractors. In this work, we focus on models with multiple scalar fields that are non-minimally coupled to the space-time Ricci curvature scalar, motivated by the expectation of a rich particle spectrum at high energies. We show that in this family of models, the single- and multi-field predictions for CMB observables are identical, as long as there exists at least one non-minimal coupling with $ξ\gg 1$. We provide simple expressions for the Hubble scale, the number of $e$-folds, and the turn rate for systems with an arbitrary number of fields and explore the statistical properties for different priors.
title Robust non-minimal attractors in many-field inflation
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2504.12406