1. Cosmogenic activation of silicon
- Author
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Saldanha, R., Thomas, R., Tsang, R. H. M., Chavarria, A. E., Bunker, R., Burnett, J. L., Elliott, S. R., Matalon, A., Mitra, P., Piers, A., Privitera, P., Ramanathan, K., and Smida, R.
- Subjects
Physics - Instrumentation and Detectors ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Nuclear Experiment - Abstract
The production of $^{3}$H, $^{7}$Be, and $^{22}$Na by interactions of cosmic-ray particles with silicon can produce radioactive backgrounds in detectors used to search for rare events. Through controlled irradiation of silicon CCDs and wafers with a neutron beam that mimics the cosmic-ray neutron spectrum, followed by direct counting, we determined that the production rate from cosmic-ray neutrons at sea level is ($112 \pm 24$) atoms/(kg day) for $^{3}$H, ($8.1 \pm 1.9 $) atoms/(kg day) for $^{7}$Be, and ($43.0 \pm 7.1 $) atoms/(kg day) for $^{22}$Na. Complementing these results with the current best estimates of activation cross sections for cosmic-ray particles other than neutrons, we obtain a total sea-level cosmic-ray production rate of ($124 \pm 24$) atoms/(kg day) for $^{3}$H, ($9.4 \pm 2.0 $) atoms/(kg day) for $^{7}$Be, and ($49.6 \pm 7.3 $) atoms/(kg day) for $^{22}$Na. These measurements will help constrain background estimates and determine the maximum time that silicon-based detectors can remain unshielded during detector fabrication before cosmogenic backgrounds impact the sensitivity of next-generation rare-event searches., Comment: 21 pages, 16 figures, 10 tables. Accepted version of the article published in Physical Review D
- Published
- 2020
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