Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
Sami Nurmi, Enrico D. Schiappacasse, Tsutomu T. Yanagida

TL;DR
This paper proposes detecting QCD axion dark matter through transient radio signals generated during encounters between neutron stars and axion minihalos around primordial black holes, offering a new detection method.
Contribution
It introduces a novel observational approach to test QCD axion dark matter via radio signatures from neutron star encounters with axion minihalos around primordial black holes.
Findings
Encounter rates suggest detectable radio signals with current telescopes.
Resonant axion-photon conversion produces line-like radio emissions.
Potential for new axion detection strategies in astrophysical observations.
Abstract
Probing the QCD axion dark matter (DM) hypothesis is extremely challenging as the axion interacts very weakly with Standard Model particles. We propose a new avenue to test the QCD axion DM via transient radio signatures coming from encounters between neutron stars (NSs) and axion minihalos around primordial black holes (PBHs). We consider a general QCD axion scenario in which the PQ symmetry breaking occurs before (or during) inflation coexisting with a small fraction of DM in the form of PBHs. The PBHs will unavoidably acquire around them axion minihalos with the typical length scale of parsecs. The axion density in the minihalos may be much higher than the local DM density, and the presence of these compact objects in the Milky Way today provides a novel chance for testing the axion DM hypothesis. We study the evolution of the minihalo mass distribution in the Galaxy accounting for…
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