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This paper investigates the Sommerfeld enhancement mechanism in dark matter annihilation as a possible explanation for the observed gamma-ray excess in the Milky Way halo. It proposes a model with a light scalar mediator that can reconcile the observed excess with constraints from other observations like dwarf spheroidal galaxies. The work is significant because it explores a specific particle physics model to address a potential dark matter signal.
Reference

A minimal model with a light CP-even scalar mediator naturally produces a velocity-dependent annihilation cross section consistent with thermal freeze-out, the Milky Way excess, and limits from dwarf spheroidal galaxies.