New scenario of QCD axion clump formation I: Linear analysis
Cosmology and Nongalactic Astrophysics
2022-03-21 v2 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
Abstract
The QCD axion acquires the potential through the non-perturbative effect of the QCD matters around the QCD phase transition. During this period, the direct interaction between the axion and the QCD matters sets in. Focusing on the impact of this direct interaction, we propose two scenarios where the fluctuation of the axion can rapidly grow, potentially leading to the formation of axion miniclusters even if the Peccei-Quinn (PQ) symmetry was already broken during inflation. The first scenario assumes that the primordial curvature perturbation at the horizon scale during the QCD epoch was significantly enhanced and the second one assumes that the initial misalignment was tuned around the hilltop of the potential.
Keywords
Cite
@article{arxiv.2111.05785,
title = {New scenario of QCD axion clump formation I: Linear analysis},
author = {Naoya Kitajima and Kazuhiro Kogai and Yuko Urakawa},
journal= {arXiv preprint arXiv:2111.05785},
year = {2022}
}
Comments
27 pages, 13 figures