A Stepping Stone Solution to the QCD Axion Isocurvature Problem
hep-ph, astro-ph.CO
Submitted: 2026-09-23
Updated: 2026-09-23
Comments: 38 pages, 7 figures
License: http://creativecommons.org/licenses/by/4.0/
The gist: We propose a ''stepping stone'' realization of the varying Peccei Quinn (PQ) scale solution to the QCD axion isocurvature problem.
Terminology
Abstract
We propose a ''stepping stone'' realization of the varying Peccei Quinn (PQ) scale solution to the QCD axion isocurvature problem. In conventional implementations, suppressing isocurvature during high scale inflation requires a large inflationary PQ scale, while the subsequent evolution toward the much smaller late time vacuum can induce parametric resonance and nonthermal restoration of the PQ symmetry. We ameliorate this tension by introducing an intermediate PQ-breaking vacuum that is reached before the end of inflation, so that the later evolution to the present day PQ scale spans only a moderate hierarchy. The vacuum structure arises radiatively: a Yukawa coupling between the PQ scalar and PQ-charged fermions drives the quartic coupling negative at high scales while keeping it positive at lower scales. A positive dimension six operator then stabilizes a large field minimum, while the positive low energy quartic together with the quadratic terms generates the intermediate vacuum. We study two mechanisms in which the rolling inflaton removes the large field minimum, either by scanning a hidden non-Abelian gauge coupling or by directly scanning the Yukawa coupling. In both cases the PQ field is released toward the intermediate vacuum during inflation, after CMB modes have exited the horizon. We exhibit benchmark regions with subdominant backreaction on the inflationary sector and suppressed vacuum tunneling, and show that the construction permits substantially less hierarchical quartic and higher-dimensional couplings than conventional realizations that depend on a varying PQ scale. The underlying logic may have analogues for extra-dimensional or string axions, where the effective axion decay constant is controlled by geometric moduli, although realizing the required intermediate vacuum in a controlled modulus potential is nontrivial.
Sources
- Axion Cosmology
- Probing a QCD String Axion with Precision Cosmological Measurements
- The landscape of QCD axion models
- Long-term dynamics of cosmological axion strings
- Axion isocurvature and the model-building problem of low-scale inflation
- CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
- Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
- The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope
- Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey
- CMB-S4 Science Book, First Edition
- CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
- Snowmass 2021 CMB-S4 White Paper
- REMOVING THE COSMOLOGICAL BOUND ON THE AXION SCALE
- Suppressing Isocurvature Perturbations of QCD Axion Dark Matter
- Diluting the inflationary axion fluctuation by a stronger QCD in the early Universe
- Axion Misalignment Driven to the Bottom
- A Step in Flux to Suppress Axion Isocurvature
- Axion cogenesis without isocurvature perturbations
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