Journal Article

Revisiting isocurvature bounds on the minimal QCD axion

Graham, Peter W., Racco, Davide

2025

Overview

A bstract The QCD axion has important connections to early universe cosmology. For example, it is often said that isocurvature limits rule out a combination of high axion decay constant, f a , and high inflationary Hubble scale, H I . High scales are theoretically motivated, so it is important to ask how robust this constraint is. We demonstrate that this constraint is naturally evaded when the quartic coupling of the complex U(1) PQ -breaking field is small (e.g. ≲ 10 −6 ). In this case, f a changes from a larger value during inflation to a smaller value in the later universe, suppressing isocurvature perturbations. Importantly, we show that in large parts of parameter space this solution is not jeopardised by overproduction of the axion through parametric resonance. The isocurvature bounds are thus dependent on UV physics. We have found that, even for the minimal QCD axion, large parts of UV parameter space at both high f a and high H I are in fact allowed, not ruled out by isocurvature constraints.

• Publisher: Springer Berlin Heidelberg,Springer Nature B.V,SpringerOpen
• Subject: Axions and ALPs / Classical and Quantum Gravitation / Constraints / Cosmology / Dark matter / Decay rate / Early Universe Particle Physics / Elementary Particles / Hypothetical particles / Parameters / Particle Nature of Dark Matter / Particle physics / Physics / Physics and Astronomy / Quantum Field Theories / Quantum Field Theory / Quantum Physics / Regular Article - Theoretical Physics / Relativity Theory / String Theory / Universe