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Observations of cosmic rays are a sensitive probe of dark matter annihilation in our Galaxy.
- In this article we present an analysis of the AMS-02 antiproton data, reducing cosmic-ray propagation uncertainties by fitting at the same time dark matter and propagation parameters.
- The result exhibits a possible hint for dark matter pointing to an annihilation cross section close to the thermal value.
- We investigate the compatibility of this signal with a dark matter interpretation of the Galactic center excess seen in the Fermi-LAT gamma-ray data and discuss implications for dark matter models.
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