Production, quality assurance and quality control of the SiPM Tiles for the DarkSide-20k Time Projection Chamber

Abstract The DarkSide-20k dark matter direct detection experiment will employ a $${21}\,\hbox {m}^{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>21</mml:mn> <mml:mspace/> <mml:msup> <mml:mtext>m</mml:mtext> <mml:mn>2</mml:mn> </mml:msup> </mml:mrow> </mml:math> silicon photomultiplier (SiPM) array, instrumenting a dual-phase 50 tonnes liquid argon Time Projection Chamber (TPC). SiPMs are arranged into modular photosensors called Tiles , each integrating 24 SiPMs onto a printed circuit board (PCB) that provides signal amplification, power distribution, and a single-ended output for simplified readout. $$16$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>16</mml:mn> </mml:mrow> </mml:math> Tiles are further grouped into Photo-Detector Units (PDUs). This paper details the production of the Tiles and the Quality Assurance and Quality Control (QA-QC) protocol established to ensure their performance and uniformity. The production and QA-QC of the Tiles are carried out at Nuova Officina Assergi (NOA), an ISO-6 clean room facility at LNGS. This process includes wafer-level cryogenic characterisation, precision die attaching, wire bonding, and extensive electrical and optical validation of each Tile. The overall production yield exceeds 83.5%, matching the requirements of the DarkSide-20k production plan. These results validate the robustness of the Tile design and its suitability for operation in a cryogenic environment.

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Journal
The European Physical Journal C
Published
2025-11-20
DOI
https://doi.org/10.1140/epjc/s10052-025-14940-1
Primary Topic
Dark Matter and Cosmic Phenomena
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article
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article

Production, quality assurance and quality control of the SiPM Tiles for the DarkSide-20k Time Projection Chamber

G. Galiński, J. H. Vossebeld, Alfiero Leoni, A. Sung et al.
The European Physical Journal C
Dark Matter and Cosmic Phenomena
article

Production, quality assurance and quality control of the SiPM Tiles for the DarkSide-20k Time Projection Chamber

G. Galiński, J. H. Vossebeld, Alfiero Leoni, A. Sung, M. Harańczyk, G. Plante, S. Pordes, P. Franchini, Tao Zhu, T. Viant, H. Frandini Gatti, C. Hidalgo, Masao Kimura, Azam Zabihi, O. Smirnov, M. Cadeddu, A. Chepurnov, A. Grobov, C. Sunny, E. Aprile, G. Fiorillo, M. Caravati, J. Monroe, Martin W. Bloem, Z. Balmforth, O. Azzolini, M. Laí, Davide Colaiuda, M. Gulino, I Sargeant, K. Nikolopoulos, P. Cavalcante, L. Lidey, P. Di Stefano, D. Rudik, Ahmed Morsy, L. Mapelli, F. Ragusa, S. Piacentini, A. Oleinik, M. G. Boulay, V. Goicoechea Casanueva, Y. P. Zhang, S. Viel, M. Morrocchi, E. Ellingwood, A Caminata, M. Lissia, A. K. Alton, P. Musico, I. F. M. Albuquerque, O. A. Taborda, V. Pesudo, C. Jillings, Aldo Ianni, V. Cocco, A. Buchowicz, Dennis L. Huff, V. N. Muratova, O. Lychagina, Tomasz Mróz, A. M. Szelc, L. Williams, S. Chashin, J. Runge, J. Maricic, John Taylor, M. Pallavicini, G. Paternoster, S. Bussino, A. Derbin, M. D’Aniello, V. Bocci, A. A. Klenin, D. Gahan, P. Amaudruz, Matteo Sestu, C. Roberts, S. Sanfilippo, G. Korga, T. Hessel, Y. Wang, A.F.V. Cortez, S. Koulosousas, W. Bonivento, M. Kuss, J. Lipp, G. Scioli, D. Santone, T. Alexander, T. Erjavec, A. Zichichi, Naomi Fearon, R. Nania, M. D. Skorokhvatov, G. Testera, Lisa Ferro, T. Braun, N. Pino, Byungwoo Park, C. Galbiati, A. Ritchie-Yates, Giovanni Grilli di Cortona, I. S. Nikulin, Giacomo Gallina, Angela Peck, F. Ragusa, L. Luzzi, O. Samoylov, L. Di Noto, S. Merzi, V. Ippolito, S. Ravinthiran, V. Stornelli, A. Kemp, A. Jamil, R. Keloth, M. Rolo, A. Taylor, P. Garcia Abia, C.J. Martoff, V. Shalamova, G. K. Giovanetti, G. Nieradka, E. Conde Vilda, K. Thieme, R. Santorelli, S. Torres-Lara, C. Dionisi, Pablo Kunzé, Roberta Calabrese, I. Ahmad, Giovanni Darbo, A. Pocar, M. Fernández Díaz, B. Vyas, F. Dordei, M. Wada, A. L. Hallin, G Rogers, A Kubankin, G. Grauso, S. Minutoli, K. Olchanski, Edivaldo Moura Santos, B. Cleveland, A. Sheshukov, M. Atzori Corona, L. Consiglio, P. Agnes, V. Oleynikov, E. Leason, K. Mavrokoridis, O. Macfadyen, Derek Fleming, P. Pralavorio, Anton M. Dainty, A. Barrado Olmedo, D. Papi, Plaban Kumar Bhowmick, A. Steri, G. Zuzel, M. Simeone, J. Nowak, S. Choudhary, S. D’Auria, B. S. Costa, Fabio Acerbi, B. Bottino, E. Scapparone, Grzegorz Pastuszak, Paolo Ventura, G. Dellacasa, T. Smirnova, F. Raffaelli, Y. Coadou, P. Salomone, A. Padmanabhan, S. Cebrián, S. Resconi, A. K. Thompson, A. Gendotti, N. Cargioli, A. Gola, Miguel Cárdenas‐Montes, G. Dolganov, A. P. D. Ramirez, R. de Asmundis, P. Zakhary, Andrea Ficorella, R. Perez, M. Walczak, E. Moretti, M. Kuźniak, M. Cadoni, L. Pandola, S. Westerdale, D. J. Auty, A. Roberts, F. Spadoni, N. Canci, M. Czubak, M. Garbini, Giacomo Matteucci, F. Gabriele, V. Camillo, E. Frolov, A. Castellani, A. Messina, E. Pantic, M. P. Zykova, J. H. Yin, S. Horikawa, S. Stracka, E.V. Hungerford, M. Ave, I. C. Avetisov, L. P. Rignanese, P. Organtini, T. Hugues, M. Kuźwa, L. Grandi, C. Mariani, A. Hamer, S. De Cecco, D. Franco, L. K. Dias, M. Angiolilli, L. Kotsiopoulou, M. Queiroga Bazetto, D. Díaz Mairena, E. Nikoloudaki, L. Romero, A. Tricomi, Aritra Mitra, M. Rossi, M. Martínez, F. Retière, I. N. Machulin, S. Blua, M. Carlini, A. L. Renshaw, E. Paoloni, E. Unzhakov, K. Pelczar, A. Rubbia, A. Marasciulli, S. Manecki, M. Gromov, A. Devoto, M. Razeti, A. Vishneva, G. Batignani, J. Busto, M. Nessi, S. M. Mari, A. Rivetti, M. Murra, S. Albergo, M. Spangenberg, E. Le Guirriec, B. C. Smith, C. Yang, N. Kemmerich, I. Manthos, L. Cifarelli, R. Tartaglia, S. Davini, A. Zani, R. B. Vogelaar, P. Skensved, M. A. Sabia, J. Hu, C. Savarese, D. A. Semenov, M. Wójcik, B. R. Hackett, Y. A. Ramachers, Y. Suvorov, K. Kondo, V. Dronik, A. Gawdzik, A. Elersich, M. La Commara, A. B. McDonald, H. O. Back, A. Órtiz de Solórzano, R. Milincic, M. Rescigno, B. Harrop, M. Van Uffelen, F. G. Schuckman, P. Adhikari, S. S. Poudel, Fabrice Hubaut, P. Barrillon, E Preosti, J Hollingham, S. Resconi, F Dylon, I Machts, Riccardo Pavarani, M. Pronesti, S Tullio
article en

Abstract

Abstract The DarkSide-20k dark matter direct detection experiment will employ a $${21}\,\hbox {m}^{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>21</mml:mn> <mml:mspace/> <mml:msup> <mml:mtext>m</mml:mtext> <mml:mn>2</mml:mn> </mml:msup> </mml:mrow> </mml:math> silicon photomultiplier (SiPM) array, instrumenting a dual-phase 50 tonnes liquid argon Time Projection Chamber (TPC). SiPMs are arranged into modular photosensors called Tiles , each integrating 24 SiPMs onto a printed circuit board (PCB) that provides signal amplification, power distribution, and a single-ended output for simplified readout. $$16$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>16</mml:mn> </mml:mrow> </mml:math> Tiles are further grouped into Photo-Detector Units (PDUs). This paper details the production of the Tiles and the Quality Assurance and Quality Control (QA-QC) protocol established to ensure their performance and uniformity. The production and QA-QC of the Tiles are carried out at Nuova Officina Assergi (NOA), an ISO-6 clean room facility at LNGS. This process includes wafer-level cryogenic characterisation, precision die attaching, wire bonding, and extensive electrical and optical validation of each Tile. The overall production yield exceeds 83.5%, matching the requirements of the DarkSide-20k production plan. These results validate the robustness of the Tile design and its suitability for operation in a cryogenic environment.

The European Physical Journal CVol. 85(11)
University of California, Riverside (US), Warsaw University of Technology (PL), Roma Tre University (IT), Belgorod National Research University (RU), Jagiellonian University (PL), Centre National de la Recherche Scientifique (FR), TRIUMF (CA), University of Hawaii System (US), D. Mendeleyev University of Chemical Technology of Russia (RU), Pacific Northwest National Laboratory (US), University of Liverpool (GB), Fort Lewis College (US), Augustana University (US), University of Alberta (CA), Universität Hamburg (DE), Istituto Nazionale di Fisica Nucleare (IT), Science and Technology Facilities Council (GB), University of Cagliari (IT), Politecnico di Torino (IT), Universidade de São Paulo (BR), Royal Holloway University of London (GB), Lodz University of Technology (PL), University of Milan (IT), Chinese Academy of Sciences (CN), Lomonosov Moscow State University (RU), Princeton University (US), University of Washington (US), Queen's University (CA), Williams College (US), Fondazione Bruno Kessler (IT), Università degli Studi di Enna Kore (IT), University of Massachusetts Amherst (US), University of Hawaii–West Oahu (US), Universidad de Zaragoza (ES), University of L'Aquila (IT), Kurchatov Institute (RU), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso (IT), Temple College (US), Laboratoire AstroParticule et Cosmologie (FR), University of California System (US), University of Manchester (GB), Joint Institute for Nuclear Research (RU), ETH Zurich (CH), University of Catania (IT), University of Warwick (GB), University of Oxford (GB), University of Chicago (US), The Edgbaston Hospital (GB), Centre de physique des particules de Marseille (FR), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), Centro Ricerche Enrico Fermi (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Catania (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Genova (IT), Fondazione Stella Maris (IT), Petersburg Nuclear Physics Institute (RU), Institut National de Physique Nucléaire et de Physique des Particules (FR), Università degli Studi Internazionali di Roma (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (IT), Institute of High Energy Physics (CN), Nicolaus Copernicus Astronomical Center (PL), Istituto Nazionale di Fisica Nucleare, Sezione di Bologna (IT), Moscow State University (TJ), Gran Sasso Science Institute (IT), Snolab (CA), Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Pisa (IT), University of Chinese Academy of Sciences (CN), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), University of Houston (US), Budker Institute of Nuclear Physics (RU), Laurentian University (CA), Carleton University (CA), Lancaster University (GB), University of Naples Federico II (IT), Columbia University (US), University of Birmingham (GB), University of Genoa (IT), University of California, Davis (US), Temple University (US), Virginia Tech (US), Sapienza University of Rome (IT), National Research Nuclear University MEPhI (RU), University of Bologna (IT), Politecnico di Milano (IT), University of Edinburgh (GB), Polish Academy of Sciences (PL)
National Science Foundation, U.S. Department of Energy, Battelle, Aix-Marseille Université, Royal Society, European Commission, Deutsche Forschungsgemeinschaft, Agence Nationale de la Recherche, Fundação de Amparo à Pesquisa do Estado de São Paulo, National Natural Science Foundation of China, Fundacja na rzecz Nauki Polskiej, Chinese Academy of Sciences, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Ministerstwo Edukacji i Nauki, Ministerio de Ciencia e Innovación, Istituto Nazionale di Fisica Nucleare, Office of Science, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, European Regional Development Fund, Labex UnivEarthS, Institut National de Physique Nucléaire et de Physique des Particules, Fermilab, Pacific Northwest National Laboratory
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Dark Matter and Cosmic Phenomena
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