English

Backgrounds in the DEAP-3600 Dark Matter Experiment

Instrumentation and Methods for Astrophysics 2018-05-17 v1 Cosmology and Nongalactic Astrophysics

Abstract

The DEAP-3600 experiment, located at SNOLAB, is searching for dark matter with a single phase liquid argon (LAr) target. For a background-free exposure of 3000 kg\cdotyr, the projected sensitivity to the spin-independent WIMP-nucleon cross section at 100 GeV/c2^2 WIMP mass is 1046^{-46} cm2^{2}. The experimental signature of dark matter interactions is keV-scale argon recoils producing 128 nm LAr scintillation photons which are wavelength shifted and observed by 255 PMTs. To reach the large background-free exposure, a combination of careful material selection, passive shielding, active vetoes, fiducialization and pulse shape discrimination (PSD) is used. The main concept of the background rejection in DEAP-3600 is the powerful PSD, employing the large difference between fast and slow components of LAr scintillation light. The designed background level of DEAP-3600 is less than 0.6 events in a 3000 kg\cdotyr exposure. The experiment was filled in November 2016 and is currently taking dark matter search data.

Keywords

Cite

@article{arxiv.1805.06073,
  title  = {Backgrounds in the DEAP-3600 Dark Matter Experiment},
  author = {B. Lehnert},
  journal= {arXiv preprint arXiv:1805.06073},
  year   = {2018}
}

Comments

Proceedings for TAUP2017

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