  Using Bogomil'nyi inequality and the vanishing of topological charge at the
unset of nucleation of a new universe permits a simpler,more direct insight
into how topological defects (kinks and anti kinks) contribute to initial
conditions at the onset of inflationary cosmology. Currently, there are few
bridges between initial conditions for cosmological inflation and the
nucleation of a new universe. This presentation shows how this can be done
while still employing Venezianos prescription for forming a link between quanta
of length, the magnitude of a dilaton field and forces gravitational and gauge
alike.
