  Holographic space-time, a theory of quantum gravity that generalizes string
theory and quantum field theory, predicts black holes in the early
matter-dominated era of its models of inflation. Before these black holes can
decay, there is a chance that enough of these particles merge to produce
radiation visible today in the Cosmic Microwave background. To discover if this
is the case, we perform a rudimentary computer simulation. We show that no
problematic black holes are formed by mergers in the Holographic Space-time
models of inflation. However, we conclude that tiny bound structures containing
black holes remnants form in this theory unconditionally. Since black hole
decay products are mostly massive standard model particles, and perhaps their
superpartners, the fate of these structures is a complicated dynamical problem
that requires further study. It suggests the possibility of primordial
structures on the order of the horizon size at the beginning of the radiation
dominated era. This is about $10^9\ L_P$ in the current model.
