  In this paper we discuss classical and quantum aspects of cosmological models
in Brans-Dicke theory. First, we review cosmological bounce solution in
Brans-Dicke theory that obeys energy conditions (without ghost) for a universe
filled with radiative fluid. Then we quantize this classical model in a
canonical way, establishing the corresponding Wheeler-DeWitt equation in the
minisuperspace, and analyze the quantum solutions. When the energy conditions
are violated, corresponding to the case $\omega<-3/2$, the energy is bounded
from below and singularity-free solutions are found. However, in the case
$\omega> -3/2$ we cannot compute the evolution of the scale factor by
evaluating the expectation values because the wave function is not finite
(energy spectrum is not bounded from below). But we can analyze this case using
Bohmian mechanics and the de Broglie-Bohm interpretation of quantum mechanics.
Using this approach, the classical and quantum results can be compared for any
value of $\omega$.
