Measurement of the bulk radioactive contamination of detector-grade silicon with DAMIC at SNOLAB

  • The Damic Collaboration
  • , A. Aguilar-Arevalo
  • , D. Amidei
  • , D. Baxter
  • , G. Cancelo
  • , B. A. Cervantes Vergara
  • , A. E. Chavarria
  • , E. Darragh-Ford
  • , J. C. D'Olivo
  • , J. Estrada
  • , F. Favela-Perez
  • , R. Gaïor
  • , Y. Guardincerri
  • , T. W. Hossbach
  • , B. Kilminster
  • , I. Lawson
  • , S. J. Lee
  • , A. Letessier-Selvon
  • , A. Matalon
  • , P. Mitra
  • A. Piers, P. Privitera, K. Ramanathan, J. Da Rocha, Y. Sarkis, M. Settimo, R. Smida, R. Thomas, J. Tiffenberg, M. Traina, R. Vilar, A. L. Virto

Research output: Contribution to journalArticlepeer-review

Abstract

We present measurements of bulk radiocontaminants in the high-resistivity silicon CCDs from the DAMIC experiment at SNOLAB. We utilize the exquisite spatial resolution of CCDs to discriminate between α and β decays, and to search with high efficiency for the spatially-correlated decays of various radioisotope sequences. Using spatially-correlated β decays, we measure a bulk radioactive contamination of 32Si in the CCDs of 140 ± 30 μBq/kg, and place an upper limit on bulk 210Pb of < 160 μBq/kg. Using similar analyses of spatially-correlated α and β decays, we set upper limits of < 11 μBq/kg (0.9 ppt) on 238U and < 7.3 μBq/kg (1.8 ppt) on 232Th in the bulk silicon. The ability of DAMIC CCDs to identify and reject spatially-coincident backgrounds, particularly from 32Si, has significant implications for the next generation of silicon-based dark matter experiments, where β's from 32Si decay will likely be a dominant background.

Original languageEnglish
Article numberP06019
JournalJournal of Instrumentation
Volume16
Issue number6
DOIs
StatePublished - Jun 2021

Keywords

  • Dark Matter detectors (WIMPs, axions, etc.)
  • Particle identification methods
  • Search for radioactive and fissile materials
  • Solid state detectors

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