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We reconsider the proposal of excited dark matter (DM) as an explanation for excess 511 keV gamma rays from positrons in the galactic center.
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D. P. Finkbeiner and N. Weiner, “Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal,” Phys. Rev. D 76
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C. Picciotto and M. Pospelov, “Unstable relics as a source of galactic positrons,” Phys. Lett. B 605
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