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Characterization of a CsI(Tl) Scintillator Coupled to a SiPM at Cryogenic Temperatures

M. Mirzakhani, R. Mahapatra, M. Platt

TL;DR

This work addresses achieving sub-keV energy sensitivity in scintillation detectors by coupling a $1~\mathrm{cm^3}$ CsI(Tl) crystal to a cryogenic SiPM readout with a custom transimpedance amplifier, evaluated from $100~\mathrm{K}$ to room temperature. The authors implement a comprehensive readout, shielding, and data-analysis strategy, including PCA-based event selection and quadratic light-yield calibration with $^{241}\mathrm{Am}$ and $^{55}\mathrm{Fe}$ sources. They observe a peak in the figure of merit at $175~\mathrm{K}$, a baseline resolution of $\sigma \approx 1~\mathrm{keV}$, and an effective energy threshold of $3~\mathrm{keV}$, demonstrating sub-keV sensitivity suitable for low-background rare-event searches. The results support potential applications in dark matter and CEvNS experiments and outline future work to improve readout by fiber-coupling and phonon–photon readout schemes.

Abstract

We report on the scintillation characterization of a 1 cm^3 CsI(Tl) crystal coupled to a 6 x 6 mm^2 SiPM read out with a custom transimpedance amplifier at cryogenic temperatures. The crystal was prepared with optical-grade surfaces and enclosed in a multi layer shielding system to suppress ambient light and background radiation. The detector response was studied at temperatures ranging from 100 K to room temperature. A figure of merit, defined as the ratio of the 59.5 keV peak position to the baseline resolution, showed a maximum at 175 K, indicating optimal photon detection efficiency. Pulse shape analysis demonstrated temperature-dependent variations in scintillation decay. At 175 K, the baseline resolution was sigma ~ 1 keV, corresponding to an effective threshold of ~ 3 keV. These results confirm the capability of the CsI(Tl) SiPM system to operate at low thresholds for rare-event searches and low-energy particle detection.

Characterization of a CsI(Tl) Scintillator Coupled to a SiPM at Cryogenic Temperatures

TL;DR

This work addresses achieving sub-keV energy sensitivity in scintillation detectors by coupling a CsI(Tl) crystal to a cryogenic SiPM readout with a custom transimpedance amplifier, evaluated from to room temperature. The authors implement a comprehensive readout, shielding, and data-analysis strategy, including PCA-based event selection and quadratic light-yield calibration with and sources. They observe a peak in the figure of merit at , a baseline resolution of , and an effective energy threshold of , demonstrating sub-keV sensitivity suitable for low-background rare-event searches. The results support potential applications in dark matter and CEvNS experiments and outline future work to improve readout by fiber-coupling and phonon–photon readout schemes.

Abstract

We report on the scintillation characterization of a 1 cm^3 CsI(Tl) crystal coupled to a 6 x 6 mm^2 SiPM read out with a custom transimpedance amplifier at cryogenic temperatures. The crystal was prepared with optical-grade surfaces and enclosed in a multi layer shielding system to suppress ambient light and background radiation. The detector response was studied at temperatures ranging from 100 K to room temperature. A figure of merit, defined as the ratio of the 59.5 keV peak position to the baseline resolution, showed a maximum at 175 K, indicating optimal photon detection efficiency. Pulse shape analysis demonstrated temperature-dependent variations in scintillation decay. At 175 K, the baseline resolution was sigma ~ 1 keV, corresponding to an effective threshold of ~ 3 keV. These results confirm the capability of the CsI(Tl) SiPM system to operate at low thresholds for rare-event searches and low-energy particle detection.

Paper Structure

This paper contains 11 sections, 9 figures.

Figures (9)

  • Figure 1: Actual picture of detector and scintillator crystal.
  • Figure 2: 3D schematic of the cryostat shielding configuration designed in AutoCAD, showing the layer sequence from inner to outer: a $0.2\,\text{mm}$ copper layer, a $5\,\text{mm}$ PLA filament, a $4\,\text{mm}$ lead sheet, and a $2\,\text{mm}$ plastic rubber enclosure.
  • Figure 3: Signal to Noise Ratio (SNR) vs. time tag of each event (triggered moment) until cooling down to 14K.
  • Figure 4: (1) Actual picture of amplifier circuit, (2) the attached SiPM to rear side of amplifier board.
  • Figure 5: Custom amplifier board designed for this project in collaboration with Atom Spectra Australia.
  • ...and 4 more figures