23–27 Jan 2023
Saha Institute of Nuclear Physics
Asia/Kolkata timezone

Alpha Quenching Factor in Liquid Argon

24 Jan 2023, 12:00
20m
Meghnad Saha Auditorium (Saha Institute of Nuclear Physics)

Meghnad Saha Auditorium

Saha Institute of Nuclear Physics

1/AF, Bidhannagar, Kolkata-700064, West Bengal, India.
Contributory Talk

Speaker

Susnata Seth (Department of Physics, Carleton University, Ottawa, Ontario, K1S 5B6, Canada and Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Queen’s University, Kingston Ontario K7L 3N6, Canada)

Description

The DEAP-3600 (Dark matter Experiment using Argon Pulseshape discrimination) experiment located at SNOLAB utilizes liquid argon as a target material. It searches for the scintillation light signal induced by Weakly Interacting Massive Particle (WIMP) candidates of dark matter via spin-independent interactions. For the DEAP-3600 detector, alpha particles are one of the intrinsic backgrounds which originate primarily from short- and long-lived radon ($^{222}$Rn) progeny. In order to identify and mitigate alpha-induced backgrounds, the quenching of alpha particles in liquid argon must be understood. In this work we performed a relative measurement of alpha quenching using scintillation light signals in the high energy region (order of MeV). We have probed the uncertainty of extrapolating the quenching factor to the low-energy region. Details of the analysis procedure and fits to Birks’ law for alpha quenching will be presented here.

Author

Susnata Seth (Department of Physics, Carleton University, Ottawa, Ontario, K1S 5B6, Canada and Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Queen’s University, Kingston Ontario K7L 3N6, Canada)

Co-authors

Mark Boulay (Department of Physics, Carleton University, Ottawa, Ontario, K1S 5B6, Canada) on behalf of the DEAP Collaboration

Presentation materials