Using the largest sample to date of TNG50 simulated galaxies plus a new phase-space scaling to match the local standard of rest, astrophysical uncertainties in dark matter direct detection limits are quantified at ~60% variation and shown to be comparable to or smaller than ton-scale detector syste
Abd El Dayemet al., (GRA VITY Collaboration), Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits, Astron
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Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Using the largest sample to date of TNG50 simulated galaxies plus a new phase-space scaling to match the local standard of rest, astrophysical uncertainties in dark matter direct detection limits are quantified at ~60% variation and shown to be comparable to or smaller than ton-scale detector syste