Characterization of CRYO ASIC for charge readout in the nEXO experiment
Z. Li, M. Yu, E. Angelico, A. Atencio, A. Gupta, P. Knauss, A. Pena-Perez, B. G. Lenardo, P. Acharya, A. Amy, A. Anker, I. J. Arnquist, J. Bane, V. Belov, T. Bhatta, A. Bolotnikov, J. Breslin, P. A. Breur, J. P. Brodsky, E. Brown, T. Brunner, B. Burnell, E. Caden, G. F. Cao

TL;DR
This paper evaluates the performance of the CRYO ASIC, a cryogenic charge readout chip, demonstrating its stability, noise performance, and operational viability in liquid xenon for the nEXO experiment.
Contribution
It presents the first comprehensive performance characterization of the CRYO ASIC operating in liquid xenon, confirming its suitability for nEXO's charge readout needs.
Findings
Achieves gain stability better than 0.2% over 24 hours
Maintains low noise levels consistent with design requirements
Operates reliably in LXe with effective boiling mitigation
Abstract
nEXO is a proposed next-generation experiment searching for the neutrinoless double beta decay of Xe using a tonne-scale liquid xenon (LXe) time projection chamber (TPC). To image the ionization signals from events in the liquid xenon, the detector will employ metallized fused-silica charge collection tiles instrumented with cryogenic application-specific integrated circuits (ASICs), referred to as CRYO ASIC, which are designed to operate directly in LXe to minimize input capacitance and pick-up noise. Here we present the performance of the CRYO ASIC mounted on an auxiliary printed circuit board and evaluated both in a cryogenic environmental chamber and in a dedicated LXe test stand. We demonstrate that the ASICs achieve the desired performance at liquid xenon temperatures, showing a gain stability better than 0.2% over 24-hour operation and reliable in-situ calibration using…
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Taxonomy
TopicsNeutrino Physics Research · Dark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research
