Analysing the Brans-Dicke solutions for the dust phase, we show that, for n
egative values of omega, they contain scenarios that display an initial sub
luminal expansion followed by an inflationary phase. This is due to a repul
sive cosmic effect. We discuss these solutions with respect to the results
of the observation of high redshift supernova as well as the age problem an
d structure formation. We establish possible connections of these solutions
with those emerging from string effective models.