INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, and Vectors
arXiv:2507.13432 · doi:10.1103/fn6k-1nlc
Abstract
The decay of light bosonic dark matter particles can produce a bright electron/positron () flux that can be strongly constrained by local Voyager observations of the direct flux, as well as 511 keV Line and X-ray continuum observations of emission. We carefully analyze the yield and resulting cosmic-ray and X-ray spectra from theoretically well-motivated light dark matter models, including: (a) electrophilic axion-like particles, (b) dark photons, (c) scalars, and (d) and vector bosons. We use the morphology and spectrum of the INTEGRAL 511 keV line data, the eROSITA X-ray continuum spectrum and the Voyager spectrum to constrain the decay lifetime and coupling of each dark matter model. We find that 511 keV observations typically set world-leading limits on bosonic dark matter decay below masses of 1 GeV, while eROSITA observations provide the strongest constraints in the range from 1--10 GeV. Finally, we forecast future limits from 21 cm line searches with next-generation HERA data.
17 pages, 10 figures. Published version on PRD
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