The Particle Astrophysics group studies dark matter and neutrinos, which respectively make up most of the mass and particle content of the universe!
Astronomical measurements indicate that ~25% of the mass in the universe is made of dark matter, particles which have never been observed on earth. This is more than 5 times as much as all the particles we do know about! Our group works on direct detection of dark matter, via dark matter particle-nucleus scattering, in ultra-sensitive detectors in terrestrial laboratories
Neutrino oscillations remain the only confirmed physics beyond the Standard Model of Particle Physics. Our group’s contributions to discovering neutrino oscillations were recognized with the 2016 Breakthrough Prize in Fundamental Physics. We work on studying the symmetry properties of neutrinos using neutrino oscillations. These may explain the matter-antimatter asymmetry of the universe, without which we wouldn’t be here!
We work on dark matter direction detection experiments at underground laboratories for particle astrophysics: SNOLAB, SURF, and LNGS. We work on neutrino oscillation experiments at J-PARC, and on detector development for future neutrino experiments at CERN. On campus, we work on detector development to apply techniques from particle astrophysics to medical physics and public health.
T2K: CP-violation and the Nature of Neutrino Oscillation
T2K (Tokai to Kamioka) is a long-baseline neutrino experiment in Japan, studying neutrino oscillations. Neutrinos are elementary particles which come in three “flavours”: electron, muon, and tau. They only interact through the weak force, and are very difficult to detect as they rarely interact with matter. As neutrinos travel, they can oscillate (change) from one flavour to another, and T2K makes precise measurements of these probabilities. In particular, T2K studies whether the probabilities of oscillations of neutrinos and antineutrinos are different. If they are, this may be linked to the matter-antimatter asymmetry problem of the early universe!
Our group works particularly on reducing the impact of systematic uncertainties by using clever techniques to understand the rare interactions of neutrinos with detectors.
DEAP: Dark Matter Direct Detection using Argon Pulse Shape Discrimination
DEAP is a dark matter direct detection experiment currently taking data in SNOLAB, 2 km underneath Sudbury, Ontario in Canada. DEAP is the largest dark matter experiment running today, with a 3.6 tonne liquid argon target. When dark matter interacts in the DEAP detector, the argon target produces a tiny flash of light. The distribution of this light in time and space are used to identify the type of particle interaction in the detector.
Our group focuses on calibration and particle identification, to distinguish candidate dark matter signal interactions from background processes that may mimic the signal. Dark matter experiments must distinguish signal from backgrounds at the level of one part per billion, or better! This means the detector response must be understood just as well; we develop this understanding using many kinds of calibration data. We also develop new statistical tools to reduce uncertainties in the dark matter search.