Warm Inflation with the Standard Model

Fuente: arXiv
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Main Authors: Berghaus, Kim V., Drewes, Marco, Zell, Sebastian
Format: Preprint
Published: 2025
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author Berghaus, Kim V.
Drewes, Marco
Zell, Sebastian
author_facet Berghaus, Kim V.
Drewes, Marco
Zell, Sebastian
contents We show for the first time that warm inflation is feasible with Standard Model (SM) gauge interactions alone. Our model consists of a minimal extension of the SM by a single scalar inflaton field with an axion-like coupling to gluons and a monomial potential. The effects of light fermions, which were previously argued to render warm inflation with the SM impossible, are alleviated by Hubble dilution of their chiral chemical potentials. Our model only features one adjustable combination of parameters and accommodates all inflationary observables. We briefly discuss implications for axion experiments, dark matter, and the strong CP-problem.
format Preprint
id arxiv_https___arxiv_org_abs_2503_18829
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Warm Inflation with the Standard Model
Berghaus, Kim V.
Drewes, Marco
Zell, Sebastian
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We show for the first time that warm inflation is feasible with Standard Model (SM) gauge interactions alone. Our model consists of a minimal extension of the SM by a single scalar inflaton field with an axion-like coupling to gluons and a monomial potential. The effects of light fermions, which were previously argued to render warm inflation with the SM impossible, are alleviated by Hubble dilution of their chiral chemical potentials. Our model only features one adjustable combination of parameters and accommodates all inflationary observables. We briefly discuss implications for axion experiments, dark matter, and the strong CP-problem.
title Warm Inflation with the Standard Model
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2503.18829