In this paper we review the hypothesis that a substantial part of the
cosmic ray flux observed above about 10(19) eV may be produced by deca
ying or annihilating topological defects left over from phase transiti
ons in the early universe at grand unification energy scales (approxim
ate to 10(16) GeV). Possible signatures of cosmic ray producing defect
models are discussed which could be tested experimentally in the near
future. We thereby focus on model independent universal spectral prop
erties of the predicted particle fluxes.