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arXiv · 2510.19547

Numerical simulations of Scalar Dark Matter Around Binary Neutron Star mergers

Rohan Srikanth·Tim Dietrich·Katy Clough
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Abstract

Binary neutron star mergers provide a laboratory for probing fundamental physics through their gravitational-wave emission and electromagnetic counterparts. In particular, they may allow us to explore signatures of physics beyond the Standard Model in strong-gravity regimes, such as those of dark matter. In this work, we investigate the dynamics of light dark matter, modeled as a minimally coupled scalar field, surrounding a binary neutron star system. Our primary focus is to assess whether the scalar field remains bound to the binary over the late inspiral-merger timescales and to determine its potential impact on observable signatures. We find that, in a range of scenarios, the scalar field forms a common cloud around the binary that does not disperse. At sufficiently high densities, this leads to measurable effects, including a dephasing of the binary inspiral, a less compact post-merger remnant, and suppression of the dynamical ejecta. For densities motivated by astrophysical considerations, however, these effects remain small and are unlikely to be detectable with current or next-generation gravitational-wave observatories.

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Rohan Srikanth, Tim Dietrich, Katy Clough. 2025-10-22. Numerical simulations of Scalar Dark Matter Around Binary Neutron Star mergers. https://arxiv.org/abs/2510.19547

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