  In this paper we have investigated the classical limit in Bohmian quantum
cosmology. It is observed that in the quantum regime where the quantum
potential is greater than the classical one, one has an expansion in terms of
negative powers of the Planck constant. But in the classical limit there are
regions having positive powers of the Planck constant, and regions having
negative powers and also regions having both. The conclusion is that the
Bohmian classical limit cannot be obtained by letting the Planck constant goes
to zero.
