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Quality assurance and quality control of the $$26~\text {m}^2$$ SiPM production for the DarkSide-20k dark matter experiment

2025· article· en· W4405900692 on OpenAlexafffund
Fabio Acerbi, P. Adhikari, P. Agnes, I. Ahmad, S. Albergo, I. F. M. Albuquerque, T. Alexander, A. K. Alton, P. Amaudruz, M. Angiolilli, E. Aprile, M. Atzori Corona, D. J. Auty, M. Ave, I. C. Avetisov, O. Azzolini, G. Batignani, Z. Balmforth, A. Barrado Olmedo, P. Barrillon, G. Batignani, Plaban Kumar Bhowmick, Martin W. Bloem, S. Blua, V. Bocci, W. Bonivento, B. Bottino, M. G. Boulay, A. Buchowicz, S. Bussino, J. Busto, M. Cadeddu, Mariano Cadoni, Roberta Calabrese, V. Camillo, A Caminata, N. Canci, A. Capra, M. Caravati, Miguel Cárdenas‐Montes, N. Cargioli, Paolo Castello, P. Cavalcante, S. Cebrián, J. Cela Ruiz, S. Chashin, A. Chepurnov, L. Cifarelli, D. Cintas, B. Cleveland, Y. Coadou, V. Cocco, Davide Colaiuda, E. Conde Vilda, L. Consiglio, B. S. Costa, M. Czubak, S. D’Auria, M. Rolo, G. Darbo, S. Davini, R. de As mundis, S. De Cecco, G. Dellacasa, A. V. Derbin, F. Di Capua, L. Di Noto, P. Di Stefano, L. K. Dias, C. Dionisi, G. Dolganov, F. Dordei, V. Dronik, A. Elersich, E. Ellingwood, T. Erjavec, Naomi Fearon, M. Fernández Díaz, A. Ficorella, G. Fiorillo, P. Franchini, D. Franco, H. Frandini Gatti, E. Frolov, F. Gabriele, D. Gahan, C. Galbiati, G. Galiski, G. Gallina, G. Gallus, M. Garbini, P. Garcia Abia, A. Gawdzik, A. Gendotti, G. K. Giovanetti, V. Goicoechea Casanueva, A. Gola, L. Grandi, G. Grauso, Giovanni Grilli di Cortona, A. Grobov, M. Gromov, M Gulino, Chengcheng Guo, B. R. Hackett, A. L. Hallin, A. Hamer, M. Harańczyk, T. Hessel, S. Horikawa, J. Hu, F. Hubaut, J. Hucker, T. Hugues, E.V. Hungerford, Aldo Ianni, G. Ippoliti, V. Ippolito, A. Jamil, C. Jillings, R. Keloth, N. Kemmerich, A. Kemp, Carlos E. Kester, Masao Kimura, K. Kondo, G. Korga, L. Kotsiopoulou, S. Koulosousas, A. Kubankin, Pablo Kunzé, M. Kuss, M. Kuźniak, M. Kuźwa, M. La Commara, M. Lai, E. Le Guirriec, E. Leason, Alfiero Leoni, L. Lidey, M. Lissia, L. Luzzi, G. Longo, O. Macfadyen, I. N. Machulin, S. Manecki, I. Manthos, A. Marasciulli, G. Margutti, S. M. Mari, C. Mariani, J. Maricic, M. Martínez, C. J. Martoff, Giacomo Matteucci, K. Mavrokoridis, Emílio Mazza, A. B. McDonald, S. Merzi, A. Messina, R. Milincic, S. Minutoli, Aritra Mitra, J. Monroe, E. Moretti, M. Morrocchi, Tomasz Mróz, V. N. Muratova, M. Murphy, M. Murra, C. Muscas, P. Musico, R. Nania, M. Nessi, G. Nieradka, K. Nikolopoulos, E. Nikoloudaki, J. Nowak, K. Olchanski, A. Oleinik, V. Oleynikov, P. Organtini, A. Ortiz de Solrzano, M. Pallavicini, L. Pandola, E. Paoloni, D. Papi, Grzegorz Pastuszak, G. Paternoster, P. A. Pegoraro, K. Pelczar, Rosana Pérez, V. Pesudo, S. Piacentini, N. Pino, G. Plante, A. Pocar, M. Poehlmann, S. Pordes, P. Pralavorio, E Preosti, M Queiroga Bazetto, F. Ragusa, Y. Ramachers, A. Ramirez, S. Ravinthiran, M. Razeti, A. L. Renshaw, M. Rescigno, S. Resconi, F. Retière, L. P. Rignanese, A. Rivetti, A. Roberts, C. Roberts, G Rogers, L. Romero, M. Rossi, A. Rubbia, D. Rudik, M. Sabia, P. Salomone, O. Samoylov, S. Sanfilippo, D. Santone, R. Santorelli, Edivaldo Moura Santos, C. Savarese, E. Scapparone, F. G. Schuckman, G. Scioli, D. A. Semenov, A. Sheshukov, M. Simeone, P. Skensved, O. Smirnov, T. Smirnova, B. Smith, A. Sotnikov, F. Spadoni, M. Spangenberg, A. Steri, V. Stornelli, C. Sunny, S. Sulis, A. Sung, Y. Suvorov, A. M. Szelc, O. A. Taborda, R. Tartaglia, Ashley Taylor, John Taylor, G. Testera, K. Thieme, A. K. Thompson, S. Torres-Lara, A. Tricomi, E. Unzhakov, M. Van Uffelen, T. Viant, S. Viel, A. Vishneva, M. Wada, J. H. Vossebeld, B. Vyas, M. Walczak, Yi Wang, H. Wang, S. Westerdale, L. Williams, R. Wojaczyski, M. Wójcik, M. Wojcik, T. Wright, Yi Xie, C. Yang, J. H. Yin, Azam Zabihi, P. Zakhary, A. Zani, Y. P. Zhang, Tao Zhu, A. Zichichi, G. Zuzel, M. P. Zykova

Bibliographic record

VenueThe European Physical Journal C · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsQueen's UniversityUniversity of AlbertaLaurentian UniversityCarleton University
FundersPacific Northwest National LaboratoryInstitut National de Physique Nucléaire et de Physique des ParticulesFermilabLabex UnivEarthSScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of ScienceMinisterio de Ciencia e InnovaciónIstituto Nazionale di Fisica NucleareMinisterstwo Edukacji i NaukiConselho Nacional de Desenvolvimento Científico e TecnológicoNational Natural Science Foundation of ChinaBattelleAgence Nationale de la RechercheEuropean Regional Development FundU.S. Department of EnergyFundacja na rzecz Nauki PolskiejEuropean CommissionChinese Academy of SciencesNational Science FoundationRoyal SocietyFundação de Amparo à Pesquisa do Estado de São Paulo
KeywordsSilicon photomultiplierDark matterProduction (economics)Quality (philosophy)Quality assuranceControl (management)PhysicsComputer scienceParticle physicsBusinessDetectorOpticsEconomicsArtificial intelligenceScintillatorMarketing

Abstract

fetched live from OpenAlex

Abstract DarkSide-20k is a novel liquid argon dark matter detector currently under construction at the Laboratori Nazionali del Gran Sasso (LNGS) of the Istituto Nazionale di Fisica Nucleare (INFN) that will push the sensitivity for Weakly Interacting Massive Particle (WIMP) detection into the neutrino fog. The core of the apparatus is a dual-phase Time Projection Chamber (TPC), filled with 50 tonnes of low radioactivity underground argon (UAr) acting as the WIMP target. NUV-HD-cryo Silicon Photomultipliers (SiPM)s designed by Fondazione Bruno Kessler (FBK) (Trento, Italy) were selected as the photon sensors covering two $$10.5~\text {m}^2$$ 10.5 m 2 Optical Planes, one at each end of the TPC, and a total of $$5~\text {m}^2$$ 5 m 2 photosensitive surface for the liquid argon veto detectors. This paper describes the Quality Assurance and Quality Control (QA/QC) plan and procedures accompanying the production of FBK NUV-HD-cryo SiPM wafers manufactured by LFoundry s.r.l. (Avezzano, AQ, Italy). SiPM characteristics are measured at 77 K at the wafer level with a custom-designed probe station. As of March 2025, 1314 of the 1400 production wafers (94% of the total) for DarkSide-20k were tested. The wafer yield is $$93.2\pm 2.5$$ 93.2 ± 2.5 %, which exceeds the 80% specification defined in the original DarkSide-20k production plan.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.011
metaresearch head score (Gemma)0.010
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.061

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0110.010
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.001
Science and technology studies0.0020.001
Scholarly communication0.0020.001
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0090.004

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.017
GPT teacher head0.289
Teacher spread0.271 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations5
Published2025
Admission routes2
Has abstractyes

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