Multiple Axions Save High-Scale Inflation
arXiv:2507.07973 · doi:10.1088/1475-7516/2025/12/014
Abstract
Many models of dark matter QCD axion requires inflation at a scale ~GeV and hence does not allow for a detectable tensor mode fluctuation. This is because the domain wall problem forces the Peccei--Quinn symmetry to be broken during the inflation and the axions to be produced by the misalignment mechanism. We point out that theories with multiple axions can evade this constraint and allow for a high-scale inflation with detectable tensor mode. It only requires a condition on the anomaly coefficients so that there is a unique minimum for the axion potential without a fine-tuning or small parameters.
18 pages, 5 figures
References in corpus (14)
- Planck 2018 results. X. Constraints on inflation
- String Axiverse
- Axions In String Theory
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Axion dark matter from topological defects
- Cosmological bounds on pseudo Nambu-Goldstone bosons
- Flaxion: a minimal extension to solve puzzles in the standard model
- Topological Dark Matter
- Dynamics of Peccei-Quinn Breaking Field after Inflation and Axion Isocurvature Perturbations
- Supernova-scope for the Direct Search of Supernova Axions
- Induced Domain Walls of QCD Axion, and Gravitational Waves
- The Quality/Cosmology Tension for a Post-Inflation QCD Axion
- Revisiting Isocurvature Bounds on the Minimal QCD Axion
- Classification of three-family flavoured DFSZ axion models that have no domain wall problem