Recent results from PAMELA and FERMI suggest an excess in the electrons and positrons cosmic-ray spectra which have been tentatively interpreted in terms of Dark Matter annihilations or decays. I will review the required properties of Dark Matter models needed in order to explain these cosmic-ray observations and I will underline possible difficulties such models have to face with. I will then show astrophysical and cosmological constraints on these interpretations.
References:
e-Print: arXiv:0905.0636 [astro-ph.HE]
e-Print: arXiv:0905.0480 [hep-ph]
e-Print: arXiv:0811.3744 [astro-ph]
e-Print: arXiv:0901.3582 [hep-ph]