Nuclear-recoil energy scale in CDMS II silicon dark-matter detectors
R. Agnese, A.J. Anderson, T. Aramaki, W. Baker, D. Balakishiyeva, S., Banik, D. Barker, R. Basu Thakur, D.A. Bauer, T. Binder, A. Borgland, M.A., Bowles, P.L. Brink, R. Bunker, B. Cabrera, D.O. Caldwell, R. Calkins, C., Cartaro, D.G. Cerdeno, H. Chagani, Y.-Y. Chang, Y. Chen

TL;DR
This paper establishes the nuclear-recoil energy scale in CDMS II silicon detectors using neutron calibration, revealing slight differences in phonon and ionization efficiencies, which minimally affect prior dark matter search results.
Contribution
It provides the first detailed calibration of nuclear-recoil energy scale in CDMS II silicon detectors using a neutron resonance method, improving the accuracy of dark matter detection.
Findings
Phonon collection efficiency for nuclear recoils is about 4.8% lower than for electron recoils.
Ionization collection efficiency is near 100% below 20 keV and decreases to about 75% at 100 keV.
Impact on previous CDMS II silicon results is minimal.
Abstract
The Cryogenic Dark Matter Search (CDMS II) experiment aims to detect dark matter particles that elastically scatter from nuclei in semiconductor detectors. The resulting nuclear-recoil energy depositions are detected by ionization and phonon sensors. Neutrons produce a similar spectrum of low-energy nuclear recoils in such detectors, while most other backgrounds produce electron recoils. The absolute energy scale for nuclear recoils is necessary to interpret results correctly. The energy scale can be determined in CDMS II silicon detectors using neutrons incident from a broad-spectrum Cf source, taking advantage of a prominent resonance in the neutron elastic scattering cross section of silicon at a recoil (neutron) energy near 20 (182) keV. Results indicate that the phonon collection efficiency for nuclear recoils is % lower than for electron recoils of the…
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