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Warm, Not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites

  • Authors: Ethan O. Nadler, Mustafa A. Amin, Risa H. Wechsler, M. Sten Delos, Andrew Benson, Vera Gluscevic

Ethan O. Nadler et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

Limits on the DM particle mass, m, versus the comoving wavenumber of field modes that dominate the DM density, k*, based on DES and PS1 MW satellite observations (solid blue line; the shaded region is excluded). The dotted line shows an extrapolation of the m ∼ k* scaling to lower k* as a visual guide; for k* < 104 Mpc−1, the scaling of our mass bound steepens to ﹩m\sim {k}_{* }^{2}﹩ (see the main text for details). Gray curves show representative theoretical relationships between m and k* motivated by the production mechanisms discussed at the end of Section 3.

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