Parametric-Resonance Production of QCD Axions

Fuente: arXiv
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Autores principales: Pirzada, Gao, Yu, Yang, Qiaoli
Formato: Preprint
Publicado: 2026
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author Pirzada
Gao, Yu
Yang, Qiaoli
author_facet Pirzada
Gao, Yu
Yang, Qiaoli
contents We demonstrate that dark matter axion production is enhanced through a natural and unavoidable mechanism: primordial temperature fluctuations periodically modulate the axion mass during the QCD phase transition, thereby triggering parametric resonance in axion field evolution. This interplay between parametric resonance and the misalignment mechanism shifts the predicted axion mass window for the observed dark matter abundance to $10^{-4}-10^{-3} \, \text{eV}$, displacing the canonical axion mass window to previously unexplored higher ranges.
format Preprint
id arxiv_https___arxiv_org_abs_2602_06922
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Parametric-Resonance Production of QCD Axions
Pirzada
Gao, Yu
Yang, Qiaoli
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
We demonstrate that dark matter axion production is enhanced through a natural and unavoidable mechanism: primordial temperature fluctuations periodically modulate the axion mass during the QCD phase transition, thereby triggering parametric resonance in axion field evolution. This interplay between parametric resonance and the misalignment mechanism shifts the predicted axion mass window for the observed dark matter abundance to $10^{-4}-10^{-3} \, \text{eV}$, displacing the canonical axion mass window to previously unexplored higher ranges.
title Parametric-Resonance Production of QCD Axions
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
url https://arxiv.org/abs/2602.06922