Dynamical friction from self-interacting dark matter

Abstract

Context. Merging compact objects such as binary black holes provide a promising probe for the physics of dark matter (DM). The gravitational waves emitted during inspiral potentially allow one to detect DM spikes around black holes. This is because the dynamical friction force experienced by the inspiralling black hole alters the orbital period and thus the gravitational wave signal. Aims. The dynamical friction arising from DM can potentially differ from the collisionless case when DM is subject to self-interactions. This paper aims to understand how self-interactions impact dynamical friction. Methods. To study the dynamical friction force, we use idealised N-body simulations, where we include self-interacting dark matter. Results. We find that the dynamical friction force for inspiralling black holes would be typically enhanced by DM self-interactions compared to a collisionless medium (ignoring differences in the DM density). At lower velocities below the sound speed, we find that the dynamical friction force can be reduced by the presence of self-interactions. Conclusions. DM self-interactions have a significant effect on the dynamical friction for black hole mergers. Assuming the Chandrasekhar formula may underpredict the deceleration due to dynamical friction.

12 pages, 13 figures + appendix, accepted for publication in A&A

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• Dynamical friction in rotating ultralight dark matter galactic cores
• Simulating realistic self-interacting dark matter models including small and large-angle scattering
• Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
• Accretion of self-interacting dark matter onto supermassive black holes