  The use of techniques from loop quantum gravity for cosmological models may
solve some difficult problems in quantum cosmology. The solutions under a
number of circumstances have been well studied. We will analyse the behaviour
of solutions in the closed model, focusing on the behaviour of a universe
containing a massless scalar field. The asymptotic behaviour of the solutions
is examined, and is used to determine requirements of the initial conditions.

General Relativity and Quantum Cosmology