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High energy electrons and positrons from annihilating dark matter can imprint unique angular anisotropies on the diffuse gamma-ray flux by inverse Compton scattering off the interstellar radiation field.
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L. Zhang, X. L. Chen, Y. A. Lei and Z. G. Si, “The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background,” Phys. Rev. D 74
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S. Ando and E. Komatsu, “Anisotropy of the cosmic gamma-ray background from dark matter annihilation,” Phys. Rev. D 73
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T. A. Porter, I. V. Moskalenko and A. W. Strong, “Inverse Compton emission from galactic supernova remnants: Effect of the interstellar radiation field,” Astrophys. J. 648
2006
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D. Hooper and S. Profumo, “Dark matter and collider phenomenology of universal extra dimensions,” Phys. Rep. 453
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P. Blasi, “The origin of the positron excess in cosmic rays,” Phys. Rev. Lett. 103
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L. Zhang, G. Sigl and J. Redondo, “Galactic Signatures of Decaying Dark Matter,” JCAP 0909
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