24–27 Mar 2025
UCLA Physics and Astronomy Building 1-425
US/Pacific timezone

Dark Matter Search Status from DEAP-3600

Not scheduled
20m
UCLA Physics and Astronomy Building 1-425

UCLA Physics and Astronomy Building 1-425

475 Portola Plaza, Los Angeles, CA 90095 darkmatter@physics.ucla.edu
Talk Non-directional direct dark matter detection

Speaker

Spencer Haskins (On behalf of the DEAP collaboration)

Description

The current status of the search for dark matter from the DEAP-3600 experiment will be presented, along with a detailed description of the analysis techniques. DEAP-3600 is a direct detection experiment that uses 3.3 tonnes of liquid argon as its target material. Located over 2 km underground at SNOLAB in Sudbury, Canada, the detector is designed to observe scintillation light from nuclear recoils induced by dark matter interactions. Pulse-shape discrimination is employed to suppress the dominant background from beta decays of argon-39. Additional backgrounds include alpha decays from the inner surface of the detector and from dust within the liquid argon, radiogenic neutrons from detector components, and Cherenkov radiation.

Author

Spencer Haskins (On behalf of the DEAP collaboration)

Presentation materials

There are no materials yet.