CERN Accelerating science

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Preprint
Report number arXiv:2412.18867
Title Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment
Author(s)

Acerbi, F. (Fond. Bruno Kessler, Trento) ; Adhikari, P. (Carleton U.) ; Agnes, P. (GSSI, Aquila ; Gran Sasso) ; Ahmad, I. (Warsaw, Copernicus Astron. Ctr.) ; Albergo, S. (INFN, Catania ; Catania U. ; Catania, CSFNSM) ; Albuquerque, I.F. (Sao Paulo U.) ; Alexander, T. (PNL, Richland) ; Alton, A.K. (Wisconsin U., River Falls) ; Amaudruz, P. (TRIUMF) ; Angiolilli, M. (GSSI, Aquila ; Gran Sasso) ; Aprile, E. (Columbia U. ; Columbia U., Astron. Astrophys.) ; Atzori Corona, M. (Cagliari U. ; INFN, Cagliari) ; Auty, D.J. (Alberta U.) ; Ave, M. (Sao Paulo U.) ; Avetisov, I.C. (Lomonosov Inst. Fine Chem. Tech.) ; Azzolini, O. (INFN, Legnaro) ; Back, H.O. (Savannah River Labs, Aiken, S.C.) ; Balmforth, Z. (Hamburg U.) ; Olmedo, A. Barrado (Madrid, CIEMAT) ; Barrillon, P. (Marseille, CPPM) ; Batignani, G. (INFN, Pisa ; Pisa U.) ; Bhowmick, P. (Oxford U., Theor. Phys. ; Rutherford) ; Bloem, M. (Rutherford) ; Blua, S. (INFN, Turin ; Polytech. Turin) ; Bocci, V. (INFN, Rome) ; Bonivento, W. (Cagliari U. ; INFN, Cagliari) ; Bottino, B. (INFN, Genoa ; Genoa U.) ; Boulay, M.G. (Carleton U.) ; Buchowicz, A. (Warsaw U. of Tech.) ; Bussino, S. (Rome III U. ; INFN, Rome3) ; Busto, J. (Marseille, CPPM) ; Cadeddu, M. (Cagliari U. ; INFN, Cagliari) ; Cadoni, M. (Cagliari U. ; INFN, Cagliari) ; Calabrese, R. (Naples U. ; INFN, Naples) ; Camillo, V. (Virginia Tech.) ; Caminata, A. (INFN, Genoa) ; Canci, N. (INFN, Naples) ; Capra, A. (TRIUMF) ; Caravati, M. (GSSI, Aquila ; Gran Sasso) ; Cardenas-Montes, M. (Madrid, CIEMAT) ; Cargioli, N. (Cagliari U. ; INFN, Cagliari) ; Carlini, M. (Gran Sasso) ; Castello, P. (Cagliari U. ; INFN, Cagliari) ; Cavalcante, P. (Gran Sasso) ; Cebrian, S. (Zaragoza U.) ; Ruiz, J. Cela (Madrid, CIEMAT) ; Chashin, S. (SINP, Moscow) ; Chepurnov, A. (SINP, Moscow) ; Cifarelli, L. (Purdue U. ; Bologna U. ; INFN, Bologna) ; Cintas, D. (Zaragoza U.) ; Cleveland, B. (Laurentian U. ; SNOLAB, Lively) ; Coadou, Y. (Marseille, CPPM) ; Cocco, V. (Cagliari U. ; INFN, Cagliari) ; Colaiuda, D. (Gran Sasso ; U. Aquila (main)) ; Vilda, E. Conde (Madrid, CIEMAT) ; Consiglio, L. (Gran Sasso) ; Costa, B.S. (Sao Paulo U.) ; Czubak, M. (Jagiellonian U.) ; D'Auria, S. (INFN, Milan ; Milan U.) ; Da Rocha Rolo, M.D. (INFN, Turin) ; Darbo, G. (INFN, Genoa) ; Davini, S. (INFN, Genoa) ; de Asmundis, R. (INFN, Naples) ; De Cecco, S. (INFN, Rome ; Rome U.) ; Dellacasa, G. (INFN, Turin) ; Derbin, A.V. (St. Petersburg, INP) ; Di Capua, F. (Naples U. ; INFN, Naples) ; Di Noto, L. (INFN, Genoa) ; Di Stefano, P. (Queen's U., Kingston) ; Dias, L.K. (Sao Paulo U.) ; Dionisi, C. (INFN, Rome ; Rome U.) ; Dolganov, G. (Kurchatov Inst., Moscow) ; Dordei, F. (Cagliari U. ; INFN, Cagliari) ; Dronik, V. (Belgorod State U.) ; Elersich, A. (UC, Davis) ; Ellingwood, E. (Queen's U., Kingston) ; Erjavec, T. (UC, Davis) ; Fearon, N. (Oxford U., Theor. Phys.) ; Diaz, M. Fernandez (Madrid, CIEMAT) ; Ficorella, A. (Fond. Bruno Kessler, Trento) ; Fiorillo, G. (Naples U. ; INFN, Naples) ; Franchini, P. (Royal Holloway, U. of London ; Lancaster U.) ; Franco, D. (APC, Paris) ; Gatti, H. Frandini (Liverpool U.) ; Frolov, E. (Novosibirsk, IYF) ; Gabriele, F. (Cagliari U. ; INFN, Cagliari) ; Gahan, D. (Cagliari U. ; INFN, Cagliari) ; Galbiati, C. (Princeton U.) ; Galiski, G. (Warsaw U. of Tech.) ; Gallina, G. (Princeton U.) ; Gallus, G. (Cagliari U. ; INFN, Cagliari) ; Garbini, M. (Enrico Fermi Ctr., Rome ; INFN, Bologna) ; Abia, P. Garcia (Madrid, CIEMAT) ; Gawdzik, A. (Manchester U.) ; Gendotti, A. (Zurich, ETH) ; Giovanetti, G.K. (Williams Coll.) ; Casanueva, V. Goicoechea (Hawaii U.) ; Gola, A. (Fond. Bruno Kessler, Trento) ; Grandi, L. (Chicago U., Astron. Astrophys. Ctr. ; Chicago U., EFI ; Chicago U., KICP) ; Grauso, G. (INFN, Naples) ; di Cortona, G. Grilli (INFN, Rome ; Rome U.) ; Grobov, A. (Kurchatov Inst., Moscow) ; Gromov, M. (SINP, Moscow) ; Gulino, M. (INFN, Catania ; Split Tech. U.) ; Guo, C. (Beijing, Inst. High Energy Phys.) ; Hackett, B.R. (PNL, Richland) ; Hallin, A. (Alberta U.) ; Hamer, A. (U. Edinburgh) ; Haranczyk, M. (Jagiellonian U.) ; Hessel, T. (APC, Paris) ; Horikawa, S. (Gran Sasso ; U. Aquila (main)) ; Hu, J. (Alberta U.) ; Hubaut, F. (Marseille, CPPM) ; Hucker, J. (Queen's U., Kingston) ; Hugues, T. (Queen's U., Kingston ; Warsaw, Copernicus Astron. Ctr.) ; Hungerford, E.V. (Houston U.) ; Ianni, A. (Princeton U.) ; Ippoliti, G. (Gran Sasso) ; Ippolito, V. (INFN, Rome) ; Jamil, A. (Princeton U.) ; Jillings, C. (Laurentian U. ; SNOLAB, Lively) ; Keloth, R. (Virginia Tech.) ; Kemmerich, N. (Sao Paulo U.) ; Kemp, A. (Rutherford) ; Kester, Carlos E. (Sao Paulo U.) ; Kimura, M. (Warsaw, Copernicus Astron. Ctr.) ; Kondo, K. (Gran Sasso ; U. Aquila (main)) ; Korga, G. (Royal Holloway, U. of London) ; Kotsiopoulou, L. (U. Edinburgh) ; Koulosousas, S. (Royal Holloway, U. of London) ; Kubankin, A. (Belgorod State U.) ; Kunze, P. (GSSI, Aquila ; Gran Sasso) ; Kuss, M. (INFN, Pisa) ; Kuźniak, M. (Warsaw, Copernicus Astron. Ctr.) ; Kuzwa, M. (Warsaw, Copernicus Astron. Ctr.) ; La Commara, M. (Naples U. ; INFN, Naples) ; Lai, M. (UC, Riverside) ; Le Guirriec, E. (Marseille, CPPM) ; Leason, E. (Oxford U., Theor. Phys.) ; Leoni, A. (Gran Sasso ; U. Aquila (main)) ; Lidey, L. (PNL, Richland) ; Lissia, M. (Cagliari U. ; INFN, Cagliari) ; Luzzi, L. (Madrid, CIEMAT) ; Lychagina, O. (Dubna, JINR) ; Macfadyen, O. (Royal Holloway, U. of London) ; Machulin, I.N. (Kurchatov Inst., Moscow ; Moscow Phys. Eng. Inst.) ; Manecki, S. (Laurentian U. ; SNOLAB, Lively ; Queen's U., Kingston) ; Manthos, I. (Hamburg U.) ; Marasciulli, A. (Gran Sasso) ; Margutti, G. (CERN) ; Mari, S.M. (Rome III U. ; INFN, Rome3) ; Mariani, C. (Virginia Tech.) ; Maricic, J. (Hawaii U.) ; Martinez, M. (Zaragoza U.) ; Martoff, C.J. (PNL, Richland ; Temple U.) ; Matteucci, G. (Naples U. ; INFN, Naples) ; Mavrokoridis, K. (Liverpool U.) ; Mazza, E. (Gran Sasso) ; McDonald, A.B. (Queen's U., Kingston) ; Merzi, S. (Fond. Bruno Kessler, Trento) ; Messina, A. (INFN, Rome ; Rome U.) ; Milincic, R. (Hawaii U.) ; Minutoli, S. (INFN, Genoa) ; Mitra, A. (Coventry U.) ; Monroe, J. (Oxford U., Theor. Phys.) ; Moretti, E. (Fond. Bruno Kessler, Trento) ; Morrocchi, M. (Pisa U. ; INFN, Pisa) ; Mroz, T. (Jagiellonian U.) ; Muratova, V.N. (St. Petersburg, INP) ; Murphy, M. (Virginia Tech.) ; Murra, M. (Columbia U. ; Columbia U., Astron. Astrophys.) ; Muscas, C. (Cagliari U. ; INFN, Cagliari) ; Musico, P. (INFN, Genoa) ; Nania, R. (INFN, Bologna) ; Nessi, M. (INFN, Rome) ; Nieradka, G. (Warsaw, Copernicus Astron. Ctr.) ; Nikolopoulos, K. (Birmingham U. ; Hamburg U.) ; Nikoloudaki, E. (APC, Paris) ; Nowak, J. (Lancaster U.) ; Olchanski, K. (TRIUMF) ; Oleinik, A. (Belgorod State U.) ; Oleynikov, V. (Novosibirsk, IYF) ; Organtini, P. (Gran Sasso ; Princeton U.) ; de Solrzano, A. Ortiz (Zaragoza U.) ; Pallavicini, M. (INFN, Genoa ; Genoa U.) ; Pandola, L. (INFN, Catania) ; Pantic, E. (UC, Davis) ; Paoloni, E. (Pisa U. ; INFN, Pisa) ; Papi, D. (Alberta U.) ; Pastuszak, G. (Warsaw U. of Tech.) ; Paternoster, G. (Fond. Bruno Kessler, Trento) ; Pegoraro, P.A. (Cagliari U. ; INFN, Cagliari) ; Pelczar, K. (Jagiellonian U.) ; Perez, R. (Sao Paulo U.) ; Pesudo, V. (Madrid, CIEMAT) ; Piacentini, S. (GSSI, Aquila ; Gran Sasso) ; Pino, N. (INFN, Catania ; Catania U. ; Catania, CSFNSM) ; Plante, G. (Columbia U. ; Columbia U., Astron. Astrophys.) ; Pocar, A. (Massachusetts U., Amherst) ; Poehlmann, M. (UC, Davis) ; Pordes, S. (Virginia Tech.) ; Pralavorio, P. (Marseille, CPPM) ; Preosti, E. (Princeton U.) ; Price, D. (Manchester U.) ; Puglia, S. (INFN, Catania ; Catania U. ; Catania, CSFNSM) ; Queiroga Bazetto, M. (Liverpool U.) ; Ragusa, F. (INFN, Milan ; Milan U.) ; Ramachers, Y. (Coventry U.) ; Ramirez, A. (Houston U.) ; Ravinthiran, S. (Liverpool U.) ; Razeti, M. (Cagliari U. ; INFN, Cagliari) ; Renshaw, A.L. (Houston U.) ; Rescigno, M. (INFN, Rome) ; Resconi, S. (INFN, Milan) ; Retiere, F. (TRIUMF) ; Rignanese, L.P. (INFN, Bologna) ; Rivetti, A. (INFN, Turin) ; Roberts, A. (Liverpool U.) ; Roberts, C. (Manchester U.) ; Rogers, G. (Birmingham U.) ; Romero, L. (Madrid, CIEMAT) ; Rossi, M. (INFN, Genoa) ; Rubbia, A. (Zurich, ETH) ; Rudik, D. (Naples U. ; INFN, Naples ; Moscow Phys. Eng. Inst.) ; Sabia, M. (INFN, Rome ; Rome U.) ; Salomone, P. (INFN, Rome ; Rome U.) ; Samoylov, O. (Dubna, JINR) ; Sanfilippo, S. (INFN, Catania) ; Santone, D. (Oxford U., Theor. Phys.) ; Santorelli, R. (Madrid, CIEMAT) ; Moura Santos, E. (Sao Paulo U.) ; Savarese, C. (CENPA, Seattle) ; Scapparone, E. (INFN, Bologna) ; II F.G. Schuckman (Queen's U., Kingston) ; Scioli, G. (Purdue U. ; Bologna U. ; INFN, Bologna) ; Semenov, D.A. (St. Petersburg, INP) ; Sheshukov, A. (Dubna, JINR) ; Simeone, M. (Naples U. ; INFN, Naples) ; Skensved, P. (Queen's U., Kingston) ; Skorokhvatov, M.D. (Kurchatov Inst., Moscow ; Moscow Phys. Eng. Inst.) ; Smirnov, O. (Dubna, JINR) ; Smirnova, T. (Kurchatov Inst., Moscow) ; Smith, B. (TRIUMF) ; Sotnikov, A. (Dubna, JINR) ; Spadoni, F. (PNL, Richland) ; Spangenberg, M. (Coventry U.) ; Stefanizzi, R. (Cagliari U. ; INFN, Cagliari) ; Steri, A. (Cagliari U. ; INFN, Cagliari) ; Stornelli, V. (Gran Sasso ; U. Aquila (main)) ; Stracka, S. (INFN, Pisa) ; Sulis, S. (Cagliari U. ; INFN, Cagliari) ; Sung, A. (Princeton U.) ; Sunny, C. (Warsaw, Copernicus Astron. Ctr.) ; Suvorov, Y. (Naples U. ; INFN, Naples ; Kurchatov Inst., Moscow) ; Szelc, A.M. (U. Edinburgh) ; Taborda, O. (GSSI, Aquila ; Gran Sasso) ; Tartaglia, R. (Gran Sasso) ; Taylor, A. (Liverpool U.) ; Taylor, J. (Liverpool U.) ; Testera, G. (INFN, Genoa) ; Thieme, K. (Hawaii U.) ; Thompson, A. (Royal Holloway, U. of London) ; Torres-Lara, S. (Houston U.) ; Tricomi, A. (INFN, Catania ; Catania U. ; Catania, CSFNSM) ; Unzhakov, E.V. (St. Petersburg, INP) ; Van Uffelen, M. (Marseille, CPPM) ; Viant, T. (Zurich, ETH) ; Viel, S. (Carleton U.) ; Vishneva, A. (Dubna, JINR) ; Vogelaar, R.B. (Virginia Tech.) ; Vossebeld, J. (Liverpool U.) ; Vyas, B. (Carleton U.) ; Wada, M. (Warsaw, Copernicus Astron. Ctr.) ; Walczak, M. (GSSI, Aquila ; Gran Sasso) ; Wang, Y. (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Wang, H. (UCLA) ; Westerdale, S. (UC, Riverside) ; Williams, L. (Lewis - Clark Coll.) ; Wojaczyski, R. (Warsaw, Copernicus Astron. Ctr.) ; Wojcik, M.M. (Jagiellonian U.) ; Wojcik, M. (Lodz, Tech. U.) ; Wright, T. (Virginia Tech.) ; Xie, Y. (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Yang, C. (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Yin, J. (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Zabihi, A. (Warsaw, Copernicus Astron. Ctr.) ; Zakhary, P. (Warsaw, Copernicus Astron. Ctr.) ; Zani, A. (INFN, Milan) ; Zhang, Y. (Beijing, Inst. High Energy Phys.) ; Zhu, T. (UC, Davis) ; Zichichi, A. (Purdue U. ; Bologna U. ; INFN, Bologna) ; Zuzel, G. (Jagiellonian U.) ; Zykova, M.P. (Lomonosov Inst. Fine Chem. Tech.)

Imprint 2024-12-25
Subject category physics.ins-det ; Detectors and Experimental Techniques
Accelerator/Facility, Experiment DarkSide 20k
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 \SI{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) (Povo, Trento, Italy) were selected as the photon sensors covering two $10.5 \text{m}^2$ Optical Planes, one at each end of the TPC, and a total of $5 \text{m}^2$ 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 May 2024, 603 of the 1400 production wafers (43% of the total) for DarkSide-20k were tested, including wafers from all 57 production Lots. The wafer yield is $93.6\pm2.5$%, which exceeds the 80% specification defined in the original DarkSide-20k production plan.
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 Запись создана 2025-01-03, последняя модификация 2025-01-20


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