Multiwavelength/Multimessenger constraints on Dark Matter

We perform a multiwavelength, multimessenger analysis of the Dark Matter intepretation of the rise in the energy spectrum of the positron ratio observed by the PAMELA satellite above 10 GeV, and other cosmic ray measurements. If standard assumptions are made for the distribution of Dark Matter and the propagation of cosmic rays, current DM models cannot explain cosmic ray measurements without violating other observational constraints.