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Testing Warm Dark Matter with Kinematics of the Smallest Galaxies

  • Authors: M. Sten Delos, Niusha Ahvazi, Andrew Benson

M. Sten Delos et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 9.

68% scatter in cusp coefficients A at fixed halo mass, shown as a function of time. The solid curves include all field halos, while the dotted curves are restricted to halos that will fall into another halo at least 100 times more massive in the next 3%–6% of a Hubble time. The dashed curve represents Equation (A2).

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