Measurement of the ionization produced by sub-keV silicon nuclear recoils in a CCD dark matter detector

A. E. Chavarria, J. I. Collar, J. R. Peña, P. Privitera, A. E. Robinson, B. Scholz, C. Sengul, J. Zhou, J. Estrada, F. Izraelevitch, J. Tiffenberg, J. R. T. de Mello Neto, and D. Torres Machado
Phys. Rev. D 94, 082007 – Published 27 October 2016

Abstract

We report a measurement of the ionization efficiency of silicon nuclei recoiling with sub-keV kinetic energy in the bulk silicon of a charge-coupled device (CCD). Nuclear recoils are produced by low-energy neutrons (<24keV) from a Sb124Be9 photoneutron source, and their ionization signal is measured down to 60 eV electron equivalent. This energy range, previously unexplored, is relevant for the detection of low-mass dark matter particles. The measured efficiency is found to deviate from the extrapolation to low energies of the Lindhard model. This measurement also demonstrates the sensitivity to nuclear recoils of CCDs employed by DAMIC, a dark matter direct detection experiment located in the SNOLAB underground laboratory.

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  • Received 11 August 2016

DOI:https://doi.org/10.1103/PhysRevD.94.082007

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

A. E. Chavarria1,*, J. I. Collar1, J. R. Peña1, P. Privitera1, A. E. Robinson1,2, B. Scholz1, C. Sengul1, J. Zhou1, J. Estrada2, F. Izraelevitch2, J. Tiffenberg2, J. R. T. de Mello Neto3, and D. Torres Machado3

  • 1Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago 60637, Illinois, United States
  • 2Fermi National Accelerator Laboratory, Batavia 60510, Illinois, United States
  • 3Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro 21.941-611, Rio de Janeiro, Brazil

  • *alvaro@kicp.uchicago.edu

See Also

Search for low-mass WIMPs in a 0.6 kg day exposure of the DAMIC experiment at SNOLAB

A. Aguilar-Arevalo et al. (DAMIC Collaboration)
Phys. Rev. D 94, 082006 (2016)

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Vol. 94, Iss. 8 — 15 October 2016

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