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The dark matter explanation of both cosmic ray positron and antiproton excesses, seen by PAMELA and recently confirmed by AMS-02, inevitably faces the contradiction with the latest FERMI/LAT data on isotropic diffuse gamma-ray background (IGRB). Here we discuss a possible solution to this problem, based on the accumulation of self-interacting dark matter component in the Galactic disk. For the same...
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