2023 CAP Congress / Congrès de l'ACP 2023

(U*) PICO-500 Overview and Calibration

21 Jun 2023, 16:45

15m

UNB Kinesiology (Rm. 214 (max. 60))

Oral Competition (Undergraduate Student) / Compétition orale (Étudiant(e) du 1er cycle) Particle Physics / Physique des particules (PPD) (PPD) W3-1 DM / Neutrino 4 | DM / Neutrino 4 (PPD)

Speaker

Michaela Robert (Queen's University)

Description

PICO-500 is a large scale bubble chamber WIMP dark matter detector in its early stages of construction underground at SNOLAB. The detector will contain ~250 litres of superheated C${}_3$F${}_8$ (freon) contained between two quartz jars. The quartz jars will sit inside a pressure vessel filled with mineral oil that will control the pressure of the active freon volume. The entire detector will be housed inside a tank of ultrapure water. PICO-500’s detection method is based on the Seitz model, in which nuclear recoiling of freon from an incoming particle results in localized boiling if the energy deposition, within a critical radius, is in excess of the Seitz threshold energy. The operating Seitz threshold of PICO-500 will be optimized for dark matter sensitivity and gamma and electron insensitivity. Muons will be vetoed using strings of photomultiplier tubes around the edges of the water tank to detect their Cherenkov light. Alphas will be discriminated from dark matter signals by the acoustic parameter (AP), which describes the acoustic power of the bubble formation, and is larger in alpha events than neutron or WIMP events. Calibration of the Seitz threshold will be done by lowering a ${}^{60}$Co gamma source into the detector through 3 separate source tubes, 2 of which feed into the water tank, and 1 of which feeds into the pressure vessel. AP calibrations will be done using runs with AmBe and/or ${}^{252}$Cf neutron sources. This talk will give an overview of PICO-500 and the methods of calibration.

Presentation materials

CAP_2023_M-Robert.pdf

CAP_2023_M-Robert.pdf

CAP_2023_M-Robert.pptx