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arXiv · 0912.0742

Robust implications on Dark Matter from the first FERMI sky gamma map

Abstract

We derive robust model-independent bounds on DM annihilations and decays from the first year of FERMI gamma-ray observations of the whole sky. These bounds only have a mild dependence on the DM density profile and allow the following DM interpretations of the PAMELA and FERMI electron/positron excesses: primary channels mu+ mu-, mu+ mu-mu+mu- or e+ e- e+ e-. An isothermal-like density profile is needed for annihilating DM. In all such cases, FERMI gamma spectra must contain a significant DM component, that may be probed in the future.

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Michele Papucci, Alessandro Strumia. 2009-12-04. Robust implications on Dark Matter from the first FERMI sky gamma map. https://doi.org/10.1088/1475-7516%2F2010%2F03%2F014

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