  Two new observations have strengthened the case for the supersymmetric nature
of the Cold Dark Matter component in our universe: First, it was shown that new
data on the nuclear abundance, B/C - and 10Be/9Be ratios constrain the
diffusion parameters in Galactic Models so strongly, that they lead to a clear
deficiency in the production of diffuse hard gamma rays, antiprotons and hard
positrons, if no anomalous sources or anomalous energy dependence of the
diffusion coefficients are postulated. Second, from the precise relic density
measurement by WMAP the WIMP annihilation cross section can be determined in a
model independent way. If the WIMPS are postulated to be the neutralinos of
Supersymmetry, then only a limited region of parameter space matches this
annihilation cross section. It is shown that the resulting positrons,
antiprotons and gamma rays from the neutralino annihilation (mainly into
b-quarks) provide the correct shape and magnitude for the missing fluxes in the
Galactic Models.
  The probability of a global fit to the galactic spectra of diffuse gamma
rays, positrons and antiprotons improves from about 10^{-8} to 0.5, if Dark
Matter, as predicted by Supersymmetry,is taken into account. This corresponds
to about 6 sigma evidence for the supersymmetric nature of Dark Matter in case
of Gaussian errors.
