Axion Misalignment Across First-Order Phase Transitions
Abstract
When the axion mass is generated during a first-order phase transition and becomes non-vanishing only inside expanding true-vacuum bubbles, the standard picture of misalignment production is qualitatively modified. Using lattice simulations in an expanding universe, we study dark matter production within such a framework and identify two distinct regimes. For rapid transitions, the onset of oscillations is delayed until bubble percolation, enhancing the relic abundance. For slower transitions, spatial gradients generated by expanding bubbles suppress the effective misalignment angle through the bubble misalignment mechanism. We derive a semi-analytical expression for the relic density that provides a unified description of both regimes and accurately reproduces the simulation results. Finally, we show how this mechanism also modifies isocurvature perturbations and the small-scale matter power spectrum, with important implications for axion minicluster formation.
Versions
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BibTeX
@misc{baltabay2026axion,
title = {{Axion Misalignment Across First-Order Phase Transitions}},
author = {Galymzhan Baltabay and Francesco D'Eramo and Ville Vaskonen},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2607.01333},
eprint = {2607.01333},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2607.01333},
}
RIS
TY - UNPB
TI - Axion Misalignment Across First-Order Phase Transitions
AU - Galymzhan Baltabay
AU - Francesco D'Eramo
AU - Ville Vaskonen
PY - 2026
DA - 2026/10/14
PB - arXiv
DO - 10.48550/arxiv.2607.01333
UR - https://arxiv.org/abs/2607.01333
AB - When the axion mass is generated during a first-order phase transition and becomes non-vanishing only inside expanding true-vacuum bubbles, the standard picture of misalignment production is qualitatively modified. Using lattice simulations in an expanding universe, we study dark matter production within such a framework and identify two distinct regimes. For rapid transitions, the onset of oscillations is delayed until bubble percolation, enhancing the relic abundance. For slower transitions, spatial gradients generated by expanding bubbles suppress the effective misalignment angle through the bubble misalignment mechanism. We derive a semi-analytical expression for the relic density that provides a unified description of both regimes and accurately reproduces the simulation results. Finally, we show how this mechanism also modifies isocurvature perturbations and the small-scale matter power spectrum, with important implications for axion minicluster formation.
ER -