Lukewarm inflation and the QCD axion
hep-ph, astro-ph.CO
Submitted: 2026-09-16
Updated: 2026-09-16
Comments: 12 pages, 5 figures
License: http://creativecommons.org/licenses/by/4.0/
The gist: We show that a late period of warm inflation, at temperatures just above the QCD scale, can dilute the abundance of the QCD axion produced by the misalignment mechanism, thus avoiding the need to
Terminology
Abstract
We show that a late period of warm inflation, at temperatures just above the QCD scale, can dilute the abundance of the QCD axion produced by the misalignment mechanism, thus avoiding the need to fine-tune the initial misalignment angle in scenarios with an axion decay constant close to the GUT scale. We develop a concrete realization of this lukewarm inflation stage involving right-handed neutrinos in 0.1 - 1 GeV mass range and an associated scalar sector, showing that coherent axion oscillations are damped during this period. In this scenario, a previously generated large baryon asymmetry may also be diluted to yield the observed value, and lukewarm inflation is followed by an early-matter era dominated by the lightest right-handed neutrino, before it decays into Standard Model states. This model can be tested via changes to the number of relativistic species and the induced small-scale enhancements of the primordial curvature power spectrum, leading to primordial black holes and scalar-induced gravitational waves.
Sources
- Dark Matter
- Baryogenesis
- Axion Cosmology
- Cosmology of axion dark matter
- Cosmological aspects of inflation in a supersymmetric axion model
- Can Decaying Particles Raise the Upperbound on the Peccei-Quinn Scale?
- Dilution of axion dark radiation by thermal inflation
- The Stochastic Axion Scenario
- The QCD Axion Window and Low Scale Inflation
- QCD axions and axionlike particles in a two-inflation scenario
- Warm Inflation
- Warm Inflation and its Microphysical Basis
- The importance of being warm (during inflation)
- The inflation trilogy and primordial black holes
- Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model
- The QCD axion, precisely
- Lattice QCD for Cosmology
- Axion Cosmology Revisited
- Thermally Induced Density Perturbations in the Inflation Era
- Warm inflation model building
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