Design and Characterization of a Phonon-Mediated Cryogenic Particle Detector with an eV-Scale Threshold and 100 keV-Scale Dynamic Range
R. Ren, C. Bathurst, Y.Y. Chang, R. Chen, C.W. Fink, Z. Hong, N.A., Kurinsky, N. Mast, N. Mishra, V. Novati, G. Spahn, H. Meyer zu Theenhausen,, S.L. Watkins, Z. Williams, M.J. Wilson, A. Zaytsev, D. Bauer, R. Bunker, E., Figueroa-Feliciano, M. Hollister, L. Hsu, P. Lukens

TL;DR
This paper reports the development of a cryogenic silicon detector with eV-scale sensitivity and a 100 keV dynamic range, suitable for dark matter and neutrino detection, achieving high energy resolution and low thresholds.
Contribution
The paper introduces a novel phonon-sensitive detector exploiting the Neganov-Trofimov-Luke effect with record low energy threshold and high resolution at cryogenic temperatures.
Findings
Achieved 2.65 eV phonon energy resolution without bias
Demonstrated 9.2 eV detection threshold with offline filtering
Calibrated energy scale up to 120 keV
Abstract
We present the design and characterization of a cryogenic phonon-sensitive 1-gram Si detector exploiting the Neganov-Trofimov-Luke effect to detect single-charge excitations. This device achieved 2.65(2)~eV phonon energy resolution when operated without a voltage bias across the crystal and a corresponding charge resolution of 0.03 electron-hole pairs at 100~V bias. With a continuous-readout data acquisition system and an offline optimum-filter trigger, we obtain a 9.2~eV threshold with a trigger rate of the order of 20~Hz. The detector's energy scale is calibrated up to 120~keV using an energy estimator based on the pulse area. The high performance of this device allows its application to different fields where excellent energy resolution, low threshold, and large dynamic range are required, including dark matter searches, precision measurements of coherent neutrino-nucleus scattering,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
