ALP dark matter coupled to EM via Chern-Simons produces secondary photons from fluctuations in a pre-existing cosmological magnetic field spectrum, with Lyman-Werner flux consistent with CMB and X-ray limits.
Spectro- spatial evolution of the CMB. Part I. Discretisa- tion of the thermalisation Green’s function,
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Secondary Production of Photons from ALP Dark Matter interacting with a Cosmological Magnetic Field
ALP dark matter coupled to EM via Chern-Simons produces secondary photons from fluctuations in a pre-existing cosmological magnetic field spectrum, with Lyman-Werner flux consistent with CMB and X-ray limits.