Mapping the Milky Way’s Dark Side

Despite uncertainties in modeling baryonic feedback, the distribution of local dark matter speeds-calculated for a dataset emulating galactic dynamics at 8.3 kpc and restricted to stellar masses between $10.60$ and $10.78$ and local standard of rest masses between $10.975$ and $11.085$-remains consistent whether those feedback parameters are varied or fixed at TNG fiducial values, and notably encompasses predictions from the Standard Halo Model, suggesting that inherent galactic variance and halo mass uncertainty dominate over the specific details of baryonic physics.

New simulations and machine learning techniques are refining our understanding of dark matter’s distribution within our galaxy, paving the way for more sensitive direct detection experiments.