Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies

TL;DR

This study uses N-body simulations to explore how interactions between stars and dark matter in ultra-faint galaxies lead to dark matter depletion, core formation, and dense stellar clusters, revealing complex dynamical phenomena.

Contribution

It demonstrates that collisional interactions can transform dark matter cusps into cores and form dense stellar clusters, bridging the dynamics of globular clusters and ultra-faint galaxies.

Findings

Dark matter is depleted from galaxy centers due to dynamical friction.

Dark matter cusps are transformed into constant-density cores.

Dense stellar clusters form with properties similar to ultra-faint galaxies.

Abstract

We use controlled N-body simulations to study the collisional exchange of energy between stars and dark matter in ultra-faint galaxies. We find that dynamical friction between stars and subsolar-mass dark matter particles results in the depletion of dark matter from the galaxies' centers, thereby transforming dark matter cusps into constant-density cores. The process is particularly effective in tidally limited galaxies with low stellar velocity dispersion. As high-mass stars sink toward the center of the dark matter halo, the dynamical-to-stellar mass ratio within the stellar half-light radius decreases monotonically. The stellar population of a dark matter-dominated galaxy is thereby compacted into a dense, baryon-dominated cluster, surrounded by a dark matter halo. Such a cluster would share the chemical composition of an ultra-faint galaxy, yet would be virtually dark matter-free within its half-light radius. We moreover find that the collisional cooling with dark matter particles provides an efficient pathway for the formation of stellar binaries in the contracting cluster. The contraction is eventually slowed down due to the decreasing central dark matter densities and the formation of stellar binaries. Our models highlight that the dynamical processes governing the faintest galaxies give rise to a rich phenomenology, blurring the line between the dynamics of globular clusters and galaxies.