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

The XENONnT experiment achieved record-breaking liquid xenon purity (below 19 ppt O2_2-equivalent) by implementing a novel two-stage purification system that combines a high-efficiency copper catalyst for initial cleanup with a low-background sintered getter alloy for sustained operation, thereby enabling over 86% electron survival across the detector's drift volume.

Original author: 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.
Published 2026-11-03
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Original author: 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, F. Marignetti, T. Marrodán Undagoitia, K. Martens, J. Masbou, S. Mastroianni, V. Mazza, J. Merz, M. Messina, A. Michel, K. Miuchi, R. Miyata, A. Molinario, S. Moriyama, M. Murra, J. Müller, K. Ni, C. T. Oba Ishikawa, U. Oberlack, K. Otsuzuki, S. Ouahada, B. Paetsch, J. Palacio, Y. Pan, Q. Pellegrini, J. Pienaar, M. Pierre, G. Plante, T. R. Pollmann, F. Pompa, A. Prajapati, L. Principe, J. Qin, A. Ravindran, A. Razeto, L. Sanchez, J. M. F. dos Santos, I. Sarnoff, G. Sartorelli, M. T. Schiller, P. Schulte, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, F. Semeria, F. N. Semler, P. Shagin, X. Shen, S. Shi, H. Simgen, Z. Song, A. Stevens, C. Szyszka, A. Takeda, Y. Takeuchi, P. -L. Tan, D. Thers, G. Trinchero, C. D. Tunnell, K. Valerius, S. Vecchi, S. Vetter, G. Volta, B. von Krosigk, C. Weinheimer, M. Weiss, D. Wenz, C. Wittweg, V. H. S. Wu, Y. Xing, D. Xu, Z. Xu, M. Yamashita, J. Yang, L. Yang, J. Ye, M. Yoshida, G. Zavattini, Y. Zhao, M. Zhong, T. Zhu

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). ✨ This is an AI-generated explanation of the paper below. It is not written or endorsed by the author. For technical accuracy, refer to the original paper. Read full disclaimer

Deep beneath the Gran Sasso mountain in Italy, a massive tank of liquid xenon waits in near-perfect silence, searching for the faintest whisper of dark matter. This substance, a heavy noble gas turned liquid by extreme cold, acts as a giant, sensitive trap. When a dark matter particle, if it exists, bumps into a xenon atom, it should create a tiny flash of light and a few free electrons. Scientists capture these signals to prove the existence of the universe's most elusive substance. However, for this experiment to work, the liquid must be incredibly pure. Even a microscopic amount of oxygen or water dissolved in the xenon acts like a sponge, stealing the free electrons before they can be counted. If the electrons vanish, the signal is lost, and the search fails. The challenge is that these impurities constantly leak out of the detector's own walls, meaning the liquid must be cleaned continuously, not just once.

The XENONnT experiment, the largest of its kind, holds 8.6 tons of this precious liquid. To keep it clean enough to detect dark matter, the researchers built a new, specialized cleaning system that circulates the liquid xenon through a series of filters while it remains in its liquid state. Unlike older methods that had to turn the xenon into gas to clean it, this new system works directly on the liquid at a frigid temperature of about 175 Kelvin. The system uses powerful pumps to push the liquid through a loop, forcing it past two different types of cleaning materials. The first type is a highly efficient catalyst designed to scrub out the vast majority of impurities quickly, ideal for when the tank is first filled or after maintenance. However, this first filter has a downside: it releases a tiny amount of radon, a radioactive gas that would create background noise and confuse the dark matter search.

To solve this, the researchers designed a two-step strategy. Once the initial heavy cleaning is done, the system switches to a second type of filter made from a special metal alloy. This second filter is slightly less efficient at removing impurities, but it is incredibly clean and does not release any radioactive gas. By using the first filter to do the heavy lifting and the second to maintain the purity, the team achieved a level of cleanliness that was previously impossible. They managed to reduce the concentration of oxygen-like impurities to less than 19 parts per trillion. At this level, more than 86 percent of the electrons generated by particle interactions survive their journey across the detector, allowing the experiment to reach its full sensitivity.

The success of this system relied on overcoming significant engineering hurdles. The pumps had to move the thick, cold liquid without introducing heat or new contaminants, so the team used motors that were magnetically coupled to the spinning parts, ensuring no metal parts touched the fluid. They also added a heat exchanger that uses liquid nitrogen to cool the xenon as it moves, preventing it from boiling or forming bubbles that could disrupt the flow. The researchers tested these components extensively, measuring how much pressure the pumps could generate and how much heat the pipes absorbed. They found that the system could run continuously, maintaining the liquid's purity for months without needing to stop.

The results of this work are now being used to guide the next generation of dark matter experiments. The team demonstrated that a liquid-phase purification system can handle the massive scale of an 8.6-ton target, a feat that was previously unproven for this type of detector. By proving that they could keep the liquid xenon pure enough to catch the faintest signals, the researchers have removed a major barrier to finding dark matter. The system is now running in the background of the XENONnT experiment, silently circulating the liquid and ensuring that every electron generated by a potential dark matter collision has a clear path to detection. This achievement not only validates the current experiment but also paves the way for even larger detectors in the future, which could hold up to 100 tons of liquid xenon and push the search for the universe's hidden mass even further.

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