The erasure of Galactic bar resonances by dark matter subhaloes

TL;DR

This paper introduces a new framework to study how dark matter subhaloes affect stellar resonances with the Galactic bar, revealing that the persistence of these resonances constrains the subhalo population and dark matter properties.

Contribution

The paper develops a novel resonance-based method to probe dark matter subhalo effects on stellar populations, linking resonance survival to the subhalo mass function.

Findings

Subhaloes with mass less than 10^7 solar masses have negligible impact on co-rotation resonances.

Full cold dark matter subhalo population could erase resonances over the Galactic bar's lifetime.

Persistence of resonances suggests local subhalo density is less than one-third of CDM expectations.

Abstract

In the context of increasing appreciation for the coupling between the Galactic bar and the halo, we introduce a new framework using stars trapped in resonance with the bar to probe the Galactic dark matter subhalo population. Since resonant stars occupy a finite width in action space, perturbations from subhaloes can shift a star's actions beyond this width, causing them to circulate out of resonance. Physically, the dark substructure in the Milky Way may dissolve, puff-up, or re-order the resonance features in the stellar halo. To explore the utility of this framework, we treat individual encounters in the impulse approximation and model their cumulative effect as diffusion in the relevant action. The resulting diffusion coefficient allows us to link the survival of resonant populations to the subhalo mass function, whose properties depend on the particle nature of dark matter. Test particle integration validates the impulse treatment for low-mass subhaloes and quantifies its regime of applicability. For a Milky Way-like bar, we find individual subhaloes with $M<10^7$ M$_{\odot}$ have negligible impact on stars in co-rotation resonance, where as the full cold dark matter (CDM) population could erase the resonance over the bar's lifetime. The persistence of resonances therefore implies a suppression of the local subhalo density to less than 1/3 of CDM expectations, consistent with tidal disruptions and previous literature. The narrow widths of higher-order resonances will increase the constraining power of this framework, and therefore motivates searches for bar-resonant halo features in observational data.