One of the models proposed for the origin of ultra high energy cosmic rays
(UHECR's) suggests that these events are the decay products of relic superh
eavy metastable particles, which we call S particles. These particles can b
e produced in the reheating period following the inflationary epoch of the
early Universe. We study this possibility and obtain constraints on some pa
rameters such as the lifetime and direct couplings of the X-particle to the
inflaton field from the requirement that they are responsible for the obse
rved UHECR flux.