New mechanism for primordial black hole formation from the QCD axion
Shuailiang Ge, Jinhui Guo, Jia Liu

TL;DR
This paper introduces a novel mechanism for primordial black hole formation via collapsing closed axion domain walls in the QCD axion model, producing PBHs that could explain certain gravitational microlensing observations.
Contribution
It proposes a new PBH formation process linked to axion domain walls that are large enough to collapse, with a fixed PBH abundance unaffected by axion parameters.
Findings
PBH abundance is about 0.9% of dark matter.
PBH masses range from 10^{-9} to 1 solar mass.
Mechanism can explain OGLE microlensing events.
Abstract
We present a new mechanism for the primordial black hole (PBH) production within the QCD axion framework. We take the case where the Peccei-Quinn symmetry breaks during inflation, resulting in a string-wall network that re-enters horizon sufficiently late. Therefore, closed axion domain walls naturally arising in the network are sufficiently large to collapse into PBHs. Our numerical simulation shows that of the total wall area is in the form of closed walls. In addition, the relic abundance of dark matter is dominantly accounted for by free axions from the collapse of open walls bounded by strings. In this framework, the abundance of PBH within dark matter is calculated to be . This fraction remains unaffected by axion parameters or the re-entering horizon temperature, as it is determined by the fixed proportion of closed walls in the network,…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
