Construction and characterisation of the DarkSide-20k veto silicon photo-multiplier tiles
Abstract
Abstract Silicon photo-multipliers (SiPMs) are state-of-the-art sensors capable of detecting a single photoelectron under cryogenic conditions, with potentially lower radioactivity than widely used photomultiplier tubes. The DarkSide-20k experiment, designed to perform direct dark matter searches using liquid argon as the target material, employs SiPM technology to detect interactions in the active detector volumes, including the central dual-phase Time Projection Chamber and the Inner and Outer Veto volumes. The vetoes are designed to discriminate against radiogenic neutron and cosmic muon backgrounds associated with the dark matter search. This paper describes the completed production and test protocols for the “Veto Tiles” (called vTiles , arrays of 24 SiPMs integrated on a printed circuit board providing the power distribution and signal amplification); 16 vTiles are grouped into “Veto Photo-Detector Units” to instrument the Inner Veto volume. Each vTile underwent detailed testing at room and cryogenic temperatures, confirming stable operation, high signal-to-noise ratio, and low radioactive contamination, demonstrating the robustness of the proposed design for cryogenic conditions. The final production yield exceeded 87%, surpassing the 80% requirement and corresponding to 1920 Veto Tiles to populate 120 Veto Photo-Detector Units, plus an additional 6% as spares.
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Authors: Fabio Acerbi, Pushparaj Adhikari, P. Agnes, Iftikhar Ahmad, S. Albergo, Ivone F.M Albuquerque, Thomas Olling Alexander, Andrew Knight Alton, Pierre-Andre Amaudruz, Gioacchino Alex Anastasi, Michele Angiolilli, Elena Aprile, D. J. Auty, Maximo Ave Pernas, O. Azzolini, Henning Olling Back, Zoe Balmforth, Ana Isabel Barrado Olmedo, Pierre Barrillon, Giovanni Batignani, Michael Bedard, Swadheen Bharat, Pritindra Bhowmick, Sofia Blua, Valerio Bocci, Walter Bonivento, Bianca Bottino, Mark G. Boulay, Titanilla Braun, Andrzej Buchowicz, Severino Bussino, Jose Busto, M. Cadeddu, Mariano Cadoni, Roberta Calabrese, Vincenzo Camillo, Alessio Caminata, Nicola Canci, Mauro Caravati, Miguel Cardenas-Montes, Nicola Cargioli, Marco Carlini, Paolo Castello, Paolo Cavalcante, S. Cebrián, Alexander Chepurnov, Sarthak Choudhary, L. Cifarelli, Yann Coadou, I. Coarasa, Valentina Cocco, Estefania Conde Vilda, Lucia Consiglio, Harrison Coombes, Andre Filipe Ventura Cortez, Barbara S Costa, Milena Czubak, S. D’Auria, Manuel Dionisio Da Rocha Rolo, Alexander Dainty, Giovanni Darbo, Stefano Davini, Riccardo De Asmundis, Sandro de Cecco, M. De Napoli, G. Dellacasa, Alexander Derbin, Lea Di Noto, Philippe Di Stefano, Daniel Diaz Mairena, Carlo Dionisi, G. Dolganov, Francesca Dordei, Aaron Elersich, E. Ellingwood, T. Erjavec, Niamh Fearon, Marta Fernández Díaz, Luca Ferro, Andrea Ficorella, Giuliana Fiorillo, Dylon Fleming, Paolo Franchini, Davide Franco, Heriques Frandini Gatti, Federico Gabriele, Devidutta Gahan, C. Galbiati, Grzegorz Galinski, Giacomo Gallina, M. Garbini, Pablo Garcia Abia, Andrzej Gawdzik, Graham Kurt Giovanetti, Alberto Gola, Luca Grandi, Gianfrancesco Grauso, Giovanni Grilli Di Cortona, Alexey Grobov, Maxim Gromov
Institutions: University of Chicago, University of Alberta, Columbia University, Universidade de São Paulo, University of Liverpool, University of Oxford, University of Manchester, Jagiellonian University, Carleton University, Universidad de Zaragoza, University of Edinburgh, Queen's University, University of Bologna, Centre National de la Recherche Scientifique, Universität Hamburg, Sapienza University of Rome, University of Naples Federico II, University of California, Davis, University of Milan, University of Pisa, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Istituto Nazionale di Fisica Nucleare, Sezione di Genova, University of Genoa, Princeton University, Virginia Tech, University of Catania, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Warsaw University of Technology, Roma Tre University, University of Cagliari, Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, Politecnico di Torino, Savannah River National Laboratory, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Istituto Nazionale di Fisica Nucleare, Sezione di Torino, ORCID, Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Research Complex at Harwell, Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Williams College, Pacific Northwest National Laboratory, Centro Ricerche Enrico Fermi, Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Fondazione Bruno Kessler, Istituto Nazionale di Fisica Nucleare, Sezione di Catania, Gran Sasso Science Institute, Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso, Nicolaus Copernicus Astronomical Center, Augustana University, Centre de physique des particules de Marseille, Laboratoire AstroParticule et Cosmologie