English

Warming up cold inflation

High Energy Physics - Phenomenology 2021-11-09 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

The axion is a well-motivated candidate for the inflaton, as the radiative corrections that spoil many single-field models are avoided by virtue of its shift symmetry. However, axions generically couple to gauge sectors. As the axion slow-rolls during inflation, this coupling can cause the production of a non-diluting thermal bath, a situation known as "warm inflation." This thermal bath can dramatically alter inflationary dynamics and observable predictions. In this paper, we demonstrate that a thermal bath can form for a wide variety of initial conditions. Furthermore, we find that axion inflation becomes warm over a large range of couplings, and explicitly map the parameter space for two axion inflation potentials. We show that in large regions of parameter space, axion inflation models once assumed to be safely "cold" are in fact warm, and must be reevaluated in this context.

Keywords

Cite

@article{arxiv.2107.07517,
  title  = {Warming up cold inflation},
  author = {William DeRocco and Peter W. Graham and Saarik Kalia},
  journal= {arXiv preprint arXiv:2107.07517},
  year   = {2021}
}

Comments

13 pages, 4 figures, published version, v3 reflects an update to an acknowledgment

R2 v1 2026-06-24T04:14:27.789Z