Neutron star -- axion star collisions in the light of multi-messenger astronomy
Tim Dietrich, Francesca Day, Katy Clough, Michael Coughlin, Jens, Niemeyer

TL;DR
This paper explores neutron star--axion star mergers through detailed simulations, analyzing potential multi-messenger signals across gravitational waves, electromagnetic emissions, and neutrinos to probe dark matter properties.
Contribution
It provides the first comprehensive simulation-based analysis of NSAS mergers and their multi-messenger signatures, offering insights into axion dark matter detection.
Findings
Potential electromagnetic and gravitational wave signals identified
Detection distances estimated for various observatories
Constraints on axion properties discussed
Abstract
Axions are increasingly favoured as a candidate particle for the dark matter in galaxies, since they satisfy the observational requirements for cold dark matter and are theoretically well motivated. Fluctuations in the axion field give rise to stable localised overdensities known as axion stars, which, for the most massive, compact cases, are potential neutron star mimickers. In principle, there are no fundamental arguments against the multi-messenger observations of GW170817/GRB170817A/AT2017gfo arising from the merger of a neutron star with a neutron star mimicker, rather than from a binary neutron star. To constrain this possibility and better understand the astrophysical signatures of a neutron star--axion star (NSAS) merger, we present in this work a detailed example case of a NSAS merger based on full 3D numerical relativity simulations, and give an overview of the many potential…
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