Search arXiv⌕ Search

arXiv · 2611.00093

The liquid-phase xenon purification system of the XENONnT dark matter experiment

Abstract

The XENONnT dark matter experiment utilizes a dual-phase time projection chamber (TPC) housed in a cryostat filled with 8.5 t of ultra-pure liquid xenon. To achieve optimal sensitivity, free electrons generated by particle interactions are required to drift across the 1.5-meter detector under an electric field. Dissolved impurities, particularly oxygen (O$_2$), can attenuate the resulting charge signal due to electron attachment. XENONnT demands an O$_2$-equivalent concentration below 100 parts per trillion (ppt) to enable its dark matter sensitivity reach. A novel liquid-phase xenon purification system was developed that continuously circulates liquid xenon through custom-designed, packed-bed sorbent purifier units at a volumetric flow rate of $\sim$2 liters per minute (L/min) at a cryogenic temperature around 175 K. With a purification time constant of approximately 25 h, the system reached the required purity within five days. The purification strategy employs a two-step approach: For an initial cleanup, a purifier based on a copper catalyst on high-surface-area alumina support (Q5) removes impurities from the liquid xenon bulk with nearly 100% efficiency, ideal for initial detector filling or after long-term maintenance. However, the high $^{222}$Rn emanation rate of the Q5 catalyst leads to increased background in the detector. In a second step, a purifier with sintered pellets of non-evaporable getter alloy (St707) ensures sustained purity with negligible background impact. The St707-based purifier exhibits a 55% efficiency, sufficient for normal operation. Following system commissioning, XENONnT achieved an O$_2$-equivalent concentration in liquid xenon below 19 ppt during its first science run. With this exceptional purity, over 86% of generated electrons survive a full drift across the TPC.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

E. Aprile, J. Aalbers, K. Abe, M. Abu Rmilah, M. Adrover, S. Ahmed Maouloud, L. Althueser, B. Andrieu, E. Angelino, D. Antón Martin, S. R. Armbruster, F. Arneodo, L. Baudis, M. Bazyk, V. Beligotti, L. Bellagamba, R. Biondi, K. Boese, R. M. Braun, G. Bruni, R. Budnik, C. Cai, C. Capelli, J. M. R. Cardoso, A. P. Cimental Chávez, A. P. Colijn, J. Conrad, J. J. Cuenca-García, H. Dai, V. D'Andrea, L. C. Daniel Garcia, M. P. Decowski, A. Deisting, C. Di Donato, P. Di Gangi, S. Diglio, K. Eitel, S. el Morabit, R. Elleboro, A. Elykov, A. D. Ferella, C. Ferrari, H. Fischer, T. Flehmke, M. Flierman, R. Frankel, D. Fuchs, W. Fulgione, C. Fuselli, F. Gao, R. Giacomobono, R. Glade-Beucke, L. Grandi, J. Grigat, A. Guerrero Ramos, M. Guida, P. Gyorgy, R. Hammann, C. Hils, L. Hoetzsch, N. F. Hood, J. Howlett, J. Huang, A. Hurhina, M. Iacovacci, Y. Itow, J. Jakob, F. Joerg, Y. Kaminaga, S. Kazama, P. Kharbanda, M. Kobayashi, D. Koke, N. Kato, K. Kooshkjalali, A. Kopec, E. Kozlova, H. Landsman, L. Levinson, A. Li, H. Li, I. Li, J. Li, K. Li, S. Li, S. Y. Li, Z. Liang, Y. -T. Lin, S. Lindemann, M. Lindner, K. Liu, M. Liu, F. Lombardi, J. A. M. Lopes, G. M. Lucchetti, T. Luce, Y. Ma, C. Macolino, G. C. Madduri, J. Mahlstedt. 2026-10-23. The liquid-phase xenon purification system of the XENONnT dark matter experiment. https://arxiv.org/abs/2611.00093

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Positron Emission Tomography with quantum-entangled Compton events: first imaging results at clinically relevant activities

In Positron Emission Tomography, a potential, yet unutilized enhancement, may come from exploiting the quantum entanglement of the annihilation quanta, inscribed in the correlation of their polarizations. To investigate this, we built a PET demonstrator capable of measuring polarization correlations of annihilation quanta by their Compton scattering, based on single-layer scintillator polarimeters. We present a detailed study of the imaging of two $^{68}$Ge line sources, 45 MBq each, to extract the spatial resolution and assess image quality. The results show that a spatial resolution of 2.5$\pm$0.1 mm is obtained using single-pixel events, while resolutions obtained with polarization-correlated Compton events range from 3.6$\pm$0.3 mm to 4.9$\pm$0.3 mm, depending on data selection criteria. We also found that the polarization-correlated Compton events exhibit up to 20% higher average signal to random background ratio compared to the single-pixel events. We also present the first imaging of the NEMA NU-4 phantom filled with a $^{68}$Ga solution of 378 MBq initial activity, successfully combining polarization-correlated events with conventional single-pixel event selection. Based on the extracted spatial resolution, signal-to-background, signal-to-noise, contrast, and contrast-to-noise ratio, we estimate that up to 10% sensitivity increase may be attained by exploiting the polarization-correlated events, while preserving a high image quality.

physics.ins-det↗

Characterization of immersed SiPM arrays in liquid scintillator between room temperature and $-30\,^{\circ}\mathrm{C}$

Liquid scintillator detectors instrumented with distributed silicon photomultiplier (SiPM) arrays can be used in compact, topology-sensitive, and low-background experiments, but the temperature dependence of SiPMs immersed directly in the scintillation medium has not been widely characterized. We report the operation of a 125-liter linear-alkylbenzene-based liquid scintillator detector read out by 125 SiPM channels immersed in the active volume, over the range from room temperature to $-30\,^{\circ}\mathrm{C}$. The detector response was measured with cosmic-ray muons, including stopping muons followed by their Michel-electron decay. Cooling from $+15\,^{\circ}\mathrm{C}$ to $-30\,^{\circ}\mathrm{C}$ reduced the SiPM dark-count rate by a factor of 13.5, increased the single-photoelectron response by 49.1%, and increased the cosmic-ray muon light yield by 16.7%. The improved photoelectron separation and baseline stability at low temperature enabled a selection of stopping-muon events, from which the effective muon lifetime was measured to be $1959\pm132\,\mathrm{ns}$, consistent with the value expected for a hydrocarbon scintillator once $μ^{-}$ capture on carbon is taken into account.

physics.ins-det↗

Residual AM and PM Noise of Selected X-Band Amplifiers

In microwave systems design, amplitude modulation (AM) noise is often ignored relative to phase modulation (PM) noise. However, in high-performance applications requiring ultra-low PM noise, AM noise becomes a critical limiting factor due to AM-to-PM conversion mechanisms. Because AM noise specifications are rarely, if ever, provided for commercial microwave components, this study characterizes the residual AM and PM noise of several 10 GHz amplifiers. We present performance data for various Heterojunction Bipolar Transistor (HBT) amplifier designs and demonstrate the noise reduction achieved through power-summed configurations. For example, a discrete-die GaAs HBT amplifier achieves residual PM noise below $-160$ dBrad$^2$/Hz and AM noise of approximately $-155$ dB/Hz at a 1 kHz offset in a quad power-summed configuration. A notable finding is that the majority of amplifier designs surveyed in this study exhibit higher AM noise relative to their PM noise, with only a few exceptions. The impact of bias supply quality on residual noise is also quantified, demonstrating that the choice of voltage regulator is a first-order design parameter below 1 kHz offset.

physics.ins-det↗