Modern-day dark matter experiments are looking for dark matter via its direct interaction with Standard model particles. DEAP-3600 (Dark matter Experiment using Argon Pulseshape discrimination) is a single-phase liquid argon (LAr)-based, direct detection dark matter experiment located 2 km underground at SNOLAB, Sudbury. DEAP is searching for dark matter via the elastic scattering of argon nuclei by dark matter particles. The detector uses 255 photomultiplier tubes (PMTs) looking at ∼3300 kg of liquid argon in a spherical vessel. The Weakly Interacting Massive Particle (WIMP) is a prime candidate for dark matter. DEAP-3600 has currently published the leading limits on WIMP-nucleon spin-independent cross section on a LAr target of 3.9 × 10 −45 cm 2 for a 100 GeV/c 2 WIMP mass at 90% confidence level. Acquiring high sensitivity for the rare, low-energy signals produced by DM-LAr interactions requires the minimization of background signals in the detector. A major source of background in DEAP is the alpha decays produced from radon progeny present in the acrylic material that composes the flow guides in the neck region of the detector. These "neck alpha" backgrounds will be mitigated by coating the neck flow guides with a slow wavelength-shifting polymeric film -pyrene-doped polystyrene (PyPS). The long time constant of PyPS helps reject neck alpha backgrounds using Pulse Shape Discrimination (PSD). A neck alpha background suppression factor of O(10 5 ) is shown to be achieved in this work. A measurement of the optical properties i the final exclusion curves included drawing the lower mass bound of the exclusion curves, for which the author wrote additional code to calculate the lower mass bound based on overburden attenuation. Appendix B is written by the author, providing analytical reasoning for why the MIMP event rate depends on the cross-sectional area of the detector rather than the volume. xi