12–17 Jun 2016
University of Ottawa
America/Toronto timezone
Welcome to the 2016 CAP Congress! / Bienvenue au congrès de l'ACP 2016!

Session

T3-5 Cosmic Frontier: Dark Matter III (PPD) / Frontière cosmique: matière sombre III (PPD)

T3-5
14 Jun 2016, 16:15
University of Ottawa

University of Ottawa

SITE Building, 800 King Edward Ave, Ottawa, ON

Presentation materials

There are no materials yet.

  1. Dr Wolfgang Rau (Queen's University)
    14/06/2016, 16:15
    Particle Physics / Physique des particules (PPD)
    Oral (Non-Student) / orale (non-étudiant)
    The Super Cryogenic Dark Matter Search (SuperCDMS) experiment uses cryogenic semiconductor detectors to search for Weakly Interacting Massive dark matter Particles (WIMPs). After more than a decade of operations of CDMS and SuperCDMS and a sequence of world leading results, the experimental setup in the Soudan underground laboratory in Minnesota is being decommissioned and SuperCDMS will move...
    Go to contribution page
  2. Jennifer Mauel (Queen's University)
    14/06/2016, 16:30
    Particle Physics / Physique des particules (PPD)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    The GIOVE (Germanium Inner-Outer Veto) detector is a highly sensitive germanium spectrometer used to screen materials for trace amounts of radioactivity. Material screening is an important aspect of the construction rare-event experiments such as GERDA and XENON, which require extremely low background levels. GIOVE is located at the Max Planck Institute for Nuclear and Particle Physics in...
    Go to contribution page
  3. Dr Gilles Gerbier (Queen's University)
    14/06/2016, 16:45
    Particle Physics / Physique des particules (PPD)
    Oral (Non-Student) / orale (non-étudiant)
    The existence of Dark Matter in our Universe is nowadays well established, however, its exact nature still remains unknown. The goal of the NEWS-SNO (New Experiments with Spheres in SNOLAB) project is to search for particle candidates in mass regions not yet accessible by existing experiments. The planned NEWS-SNO detector consists of a spherical TPC (time-projection-chamber) out of ultrapure...
    Go to contribution page
  4. Michael Clark (Queen's University)
    14/06/2016, 17:00
    Particle Physics / Physique des particules (PPD)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    Pyrene is an interesting material because of its wavelength shifting properties. When irradiated with ultraviolet light, pyrene will emit light in the visible wavelengths. This property could be useful for experiments looking to observe scintillation light from noble gases such as argon and neon, which are popular target materials for dark matter direct detection experiments. Noble gases...
    Go to contribution page
  5. Mr Matthew Stukel (Queens University)
    14/06/2016, 17:15
    Particle Physics / Physique des particules (PPD)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    Enigmatic dark matter is responsible for 26% of the total mass-energy in the known universe. Since 1997, the DAMA/LIBRA experiment has claimed to have the first direct evidence for the observation of dark matter. One major source of background for this experiment is the 40K isotope. The chemical similarity between potassium and sodium is why trace amounts can be found in the NaI...
    Go to contribution page
Building timetable...