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

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Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment. / The DarkSide-20k Collaboration ; Franchini, P.; Nowak, J.
In: European Physical Journal C: Particles and Fields, 16.04.2025.

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The DarkSide-20k Collaboration, Franchini P, Nowak J. Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment. European Physical Journal C: Particles and Fields. 2025 Apr 16.

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@article{885bf37079c040328b50c88b33a573ab,
title = "Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment",
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. ",
keywords = "physics.ins-det",
author = "{The DarkSide-20k Collaboration} and F. Acerbi and P. Adhikari and P. Agnes and I. Ahmad and S. Albergo and Albuquerque, {I. F.} and T. Alexander and Alton, {A. K.} and P. Amaudruz and Aprile, {M. Angiolilli E.} and Corona, {M. Atzori} and Auty, {D. J.} and M. Ave and Avetisov, {I. C.} and O. Azzolini and Back, {H. O.} and Z. Balmforth and Olmedo, {A. Barrado} and P. Barrillon and G. Batignani and P. Bhowmick and M. Bloem and S. Blua and V. Bocci and W. Bonivento and B. Bottino and Boulay, {M. G.} and A. Buchowicz and S. Bussino and J. Busto and M. Cadeddu and M. Cadoni and R. Calabrese and V. Camillo and A. Caminata and N. Canci and A. Capra and M. Caravati and M. Cardenas-Montes and N. Cargioli and M. Carlini and P. Castello and P. Cavalcante and S. Cebrian and Ruiz, {J. Cela} and S. Chashin and A. Chepurnov and L. Cifarelli and P. Franchini and J. Nowak",
year = "2025",
month = apr,
day = "16",
language = "English",
journal = "European Physical Journal C: Particles and Fields",
issn = "1434-6044",
publisher = "SPRINGER",

}

RIS

TY - JOUR

T1 - Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment

AU - The DarkSide-20k Collaboration

AU - Acerbi, F.

AU - Adhikari, P.

AU - Agnes, P.

AU - Ahmad, I.

AU - Albergo, S.

AU - Albuquerque, I. F.

AU - Alexander, T.

AU - Alton, A. K.

AU - Amaudruz, P.

AU - Aprile, M. Angiolilli E.

AU - Corona, M. Atzori

AU - Auty, D. J.

AU - Ave, M.

AU - Avetisov, I. C.

AU - Azzolini, O.

AU - Back, H. O.

AU - Balmforth, Z.

AU - Olmedo, A. Barrado

AU - Barrillon, P.

AU - Batignani, G.

AU - Bhowmick, P.

AU - Bloem, M.

AU - Blua, S.

AU - Bocci, V.

AU - Bonivento, W.

AU - Bottino, B.

AU - Boulay, M. G.

AU - Buchowicz, A.

AU - Bussino, S.

AU - Busto, J.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Calabrese, R.

AU - Camillo, V.

AU - Caminata, A.

AU - Canci, N.

AU - Capra, A.

AU - Caravati, M.

AU - Cardenas-Montes, M.

AU - Cargioli, N.

AU - Carlini, M.

AU - Castello, P.

AU - Cavalcante, P.

AU - Cebrian, S.

AU - Ruiz, J. Cela

AU - Chashin, S.

AU - Chepurnov, A.

AU - Cifarelli, L.

AU - Franchini, P.

AU - Nowak, J.

PY - 2025/4/16

Y1 - 2025/4/16

N2 - 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.

AB - 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.

KW - physics.ins-det

M3 - Journal article

JO - European Physical Journal C: Particles and Fields

JF - European Physical Journal C: Particles and Fields

SN - 1434-6044

ER -