  This work compares cosmological matching conditions used in approximating
generic pre-inflationary phases of the universe. We show that the joining
conditions for primordial scalar perturbations assumed by Contaldi et al. are
inconsistent with the physically motivated Israel junction conditions, however;
performing general relativistic matching with the aforementioned constraints
results in unrealistic primordial power spectra. Eliminating the need for
ambiguous matching, we look at an alternative semi-analytic model for producing
the primordial power spectrum allowing for finite duration cosmological phase
transitions.
