  We present the energy spectra of the fluxes of positrons, anti-protons and
photons generated by Dark Matter annihilations in our galaxy, as univocally
predicted by the model of Minimal Dark Matter. Due to multi-TeV masses and to
the Sommerfeld enhancement of the annihilation cross section, distinctive
signals are generated above the background, even with a modest astrophysical
boost factor, in the range of energies soon to be explored by cosmic ray
experiments.
