Shaping the Milky Way. II. The dark matter halo's response to the LMC's passage in a cosmological context

TL;DR

This paper investigates how the Milky Way's dark matter halo responds to the passage of the Large Magellanic Cloud using cosmological simulations, revealing characteristic dynamical signatures that can inform about the galaxy's structure and dark matter physics.

Contribution

It introduces a method using basis function expansions to analyze halo responses in simulations, linking observable signatures to galaxy and dark matter properties.

Findings

Halo responds with a dipole and quadrupole pattern after LMC infall.

Dipole amplitude scales with the square of the MW-LMC mass ratio.

Timing of responses correlates with the LMC's pericenter passage.

Abstract

The distribution of dark matter in the Milky Way (MW) is expected to exhibit a large-scale dynamical response to the recent infall of the LMC. This event produces a dynamical friction wake and shifts the MW's halo density center. The structure of this response encodes information about the LMC- MW mass ratio, the LMC's orbit, the MW halo's pre-infall structure and could provide constraints on dark matter physics. To extract this information, a method to separate these effects and recover the initial shape of the MW's halo is required. Here, we use basis function expansions to analyze the halo response in eighteen simulations of MW-LMC-like interactions from the MWest cosmological, dark-matter-only zoom-in simulations. The results show that mergers similar to the LMC consistently generate a significant dipole and a secondary quadrupole response in the halo. The dipole arises from the host density center displacement and halo distortions, and its amplitude scales as the square of the MW-LMC mass ratio, peaking 0.2-0.7 Gyr after the LMC's pericenter. The quadrupole's strength depends primarily on the original axis ratios of the host halo, though contributions from the dynamical friction wake cause it to peak less than 0.3 Gyr before pericenter. Future measurements of both the dipole and quadrupole imprints of the LMC's passage in the density of the MW's stellar halo should be able to disentangle these effects and provide insight into the initial structure of the MW's halo, the MW's response, and the mass of the LMC.