The growing trove of precision astrometric observations from the Gaia space telescope and
other surveys is revealing the structure and dynamics of the Milky Way in ever more …

The properties of low-mass dark matter (DM) halos appear to be remarkably diverse relative
to cold, collisionless DM predictions, even in the presence of baryons. We show that self …

Core formation and runaway core collapse in models with self-interacting dark matter (SIDM)
significantly alter the central density profiles of collapsed haloes. Using a forward modelling …

We perform a high-resolution cosmological zoom-in simulation of a Milky Way (MW)–like
system, which includes a realistic Large Magellanic Cloud analog, using a large differential …

Self-interacting dark matter (SIDM) cosmologies admit an enormous diversity of dark matter
(DM) halo density profiles, from low-density cores to high-density core-collapsed cusps. The …

It has been proposed that gravothermal collapse due to dark matter self-interactions (ie self-
interacting dark matter, SIDM) can explain the observed diversity of the Milky Way (MW) …

We explore the properties of Milky Way (MW) subhaloes in self-interacting dark matter
models for moderate cross-sections of 1–5 cm2 g− 1 using high-resolution zoom-in N-body …

The scale-free gravothermal fluid formalism has long proved effective in describing the
evolution of self-interacting dark matter halos with a constant dark matter particle cross …

We present a suite of baryonic cosmological zoom-in simulations of self-interacting dark
matter (SIDM) haloes within the 'Feedback In Realistic Environment'(FIRE) project. The three …

The non-linear process of cosmic structure formation produces gravitationally bound
overdensities of dark matter known as halos. The abundances, density profiles, ellipticities …