Feb 15–18, 2024
Mt. Bromont
Canada/Eastern timezone

Session

Evening 3 - Feb. 16, 2024

Feb 16, 2024, 9:00 p.m.
(Mt. Bromont)

Mt. Bromont

90 Stanstead St., Bromont, J2L 1K6

Conveners

Evening 3 - Feb. 16, 2024

  • Heather Russell (University of Victoria)

Presentation materials

There are no materials yet.

  1. Michaela Robert (Queen's University)
    2024-02-16, 9:00 p.m.
    Dark Matter Searches
    Contributed Oral

    PICO-500 is a WIMP dark matter bubble chamber detector in its early stages of construction underground at SNOLAB. It is the upscaled successor of PICO-40L, which is currently operational with the objective of detecting dark matter or improving the world leading spin-dependent WIMP search limits set by PICO-60 in 2016. PICO-500 will have almost an order of magnitude greater sensitivity with a...

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  2. Emily Adams (Queen's University)
    2024-02-16, 9:15 p.m.
    Dark Matter Searches
    Contributed Oral

    The PICO collaboration searches for dark matter using superheated C3F8 in bubble chamber technology. The results of the operation of the PICO-60 detector at SNOLAB set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section.
    PICO-500 is the next-generation detector produced by PICO with a 250 kg live volume....

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  3. Tyler Reynolds (University of Toronto)
    2024-02-16, 9:30 p.m.
    Dark Matter Searches
    Contributed Oral

    The SuperCDMS collaboration uses cryogenic silicon and germanium detectors to directly search for dark matter. Among the full payload of 24 detectors are 12 HV detectors. These utilize a bias voltage across the crystal substrate to amplify the phonon signal created from particle energy depositions. We have operated 4 Ge and 2 Si HV detectors in a deep underground environment for the first time...

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  4. Ata Sattari (University of Toronto)
    2024-02-16, 9:45 p.m.
    Dark Matter Searches
    Contributed Oral

    SuperCDMS SNOLAB will be a direct detection experiment with world-leading sensitivity to low-mass dark matter (DM) that employs cryogenic silicon and germanium calorimeters. SNOLAB detectors are expected to exhibit a non-linear energy response, necessitating calibration signatures across the entire energy range of interest. A calibration method proposed for silicon-based detectors is to use...

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