The DEAP-3600 Detector and Recent Developments at SNOLAB

          @misc{ scivideos_PIRSA:11030112,
            doi = {10.48660/11030112},
            url = {https://pirsa.org/11030112},
            author = {Jillings, Christopher},
            keywords = {Particle Physics},
            language = {en},
            title = {The DEAP-3600 Detector and Recent Developments at SNOLAB},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {mar},
            note = {PIRSA:11030112 see, \url{https://scivideos.org/pirsa/11030112}}
          }
          

Abstract

The DEAP-3600 single-phase liquid-argon dark matter detector is under construction at SNOLAB. The fundamental goal of the design is to increase the volume of the detector while having the liquid argon contact the smallest possible surface comprising only clean acrylic and wavelength shifter. Specifically DEAP-3600 is a spherical detector with a 1000 kg fiducial mass and a design background rate less than 0.1 events in the WIMP region of interest in three years of data taking. Design sensitivity to WIMP dark matter at 100 GeV is 10-46 cm2. In order to achieve this ambitious goal an extensive program of background reduction and control is underway for all detector components including the acrylic vessel, process system, photomultiplier tubes and TPB wavelength shifter. Efforts to obtain acrylic with bulk Uranium and Thorium contamination below 0.3 and 1.3 ppt respectively and Pb-210 contamination below 1.1x10-8 ppt will be described. A resurfacer is under development to ensure that the surface contamination of acrylic is removed. Even with these stringent controls fiducialization will be required to reduce surface backgrounds by a factor of 1000. Preliminary studies are promising. We have operated the DEAP-1 prototype detector underground at SNOLAB; results from the DEAP-1 runs will be discussed and the impact of those runs on DEAP-3600 will be discussed. SNOLAB has recently made the “phase 2” expansion (including the cryopit and two drifts) part of the clean space. A photo essay showing recent progress in the facility and the experimental program will be presented.