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[en] The decay of dark matter is predicted by many theoretical models and can produce ob- servable contributions to the cosmic-ray fluxes. I shortly discuss the interpretation of the positron and electron excess as observed by PAMELA and Fermi LAT in terms of decaying dark matter, and I point out the implications for the Fermi LAT observations of the γ-ray flux with emphasis on its dipole-like anisotropy. (orig.)
Source
Oct 2009; 4 p; ISSN 0418-9833; 