  We study oscillatory universes within the context of Loop Quantum Cosmology.
We make a comparative study of flat and positively curved universes sourced by
scalar fields with either positive or negative potentials. We investigate how
oscillating universes can set the initial conditions for successful slow-roll
inflation, while ensuring that the semi-classical bounds are satisfied. We
observe rich oscillatory dynamics with negative potentials, although it is
difficult to respect the semi-classical bounds in models of this type.
