Abstract
A Friedmann-Robertson-Walker (FRW) model is studied in the new scalar-tensor theory of gravitation proposed by Schmidt et al. There is an assumption of a particular functional relationship between the cosmological expansion factor of the FRW model and the scalar field. Exact solutions are given, and it is observed that at least in one case $k=\ensuremath{-}1$ it is possible to obtain a model with oscillation between finite limits.
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