Naturally occurring $^{32}$Si and low-background silicon dark matter detectors
J.L. Orrell, I.J. Arnquist, M. Bliss, R. Bunker, Z.S. Finch

TL;DR
This paper investigates the sources and mitigation strategies for the radioactive isotope $^{32}$Si in silicon used for dark matter detectors, proposing methods to produce low-$^{32}$Si$ silicon and emphasizing the need for assay development.
Contribution
It identifies the variability of $^{32}$Si in commercial silicon, reviews potential source materials, and proposes analytic methods for quantifying $^{32}$Si content in silicon production.
Findings
$^{32}$Si$ levels vary with silicon source and refining history.
Feasibility of producing low-$^{32}$Si$ silicon detectors is demonstrated.
Assay methods are needed for quality assurance in silicon detector production.
Abstract
The naturally occurring radioisotope Si represents a potentially limiting background in future dark matter direct-detection experiments. We investigate sources of Si and the vectors by which it comes to reside in silicon crystals used for fabrication of radiation detectors. We infer that the Si concentration in commercial single-crystal silicon is likely variable, dependent upon the specific geologic and hydrologic history of the source (or sources) of silicon "ore" and the details of the silicon-refinement process. The silicon production industry is large, highly segmented by refining step, and multifaceted in terms of final product type, from which we conclude that production of Si-mitigated crystals requires both targeted silicon material selection and a dedicated refinement-through-crystal-production process. We review options for source material…
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