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Signatures of dark matter in celestial objects have become of increasinginterest due to their powerful detection prospects. To test any of thesesignatures, the fundamental quantity needed is the rate in which dark matter iscaptured by celestial objects. Depending on whether dark matter is light,heavy, or comparable in mass to the celestial-body scattering targets, thereare different considerations when calculating the capture rate. Furthermore, ifdark matter has strong or weak interactions, the physical behaviour importantfor capture varies. Using both analytic approximations and simulations, wedemonstrate how to treat dark matter capture in a range of celestial objectsfor arbitrary dark matter mass and interaction strength. We release ourcalculation framework as a public package available in both Python andMathematica versions, called Asteria.

Dark Matter Capture in Celestial Objects: Treatment Across Kinematic and Interaction Regimes