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Study of cosmogenic activation above ground for the DarkSide-20k experiment

Title: Study of cosmogenic activation above ground for the DarkSide-20k experiment
Authors: Agnes, Paolo; Ahmad, Iftikhar; Albergo, Sebastiano; Albuquerque, Ivone; Alexander, T.; Alton, A.K.; Amaudruz, P.; Atzori Corona, Mattia; Ave, M.; Avetisov, I.Ch.; Azzolini, Oscar; Back, Henning; Balmforth, Zoe; Barrado-Olmedo, A.; Barrillon, P.; Basco, A.; Batignani, Giovanni; Bocci, Valerio; Bonivento, Walter M.; Bottino, Bianca; Boulay, M.G.; Busto, Jose; Cadeddu, Matteo; Caminata, Alessio; Canci, Nicola; Capra, Andrea; Caprioli, S.; Caravati, M.; Cargioli, Nicola; Carlini, Marco; Casanueva, V. Goicoechea; Castello, P.; Cavalcante, P.; Cavuoti, Stefano; Cebrian, S.; Chashin, S.; Chepurnov, A.; Chyhyrynets, Eduard; Cifarelli, Luisa; Cintas, D.; Citterio, Mauro; Cleveland, B.; Cocco, V.; Colaiuda, D.; Consiglio, Lucia; Copello, Simone; Covone, Giovanni; Czubak, M.; D'Aniello, M.; D'Auria, Saverio; Da Rocha Rolo, Manuel Dionisio; Davini, Stefano; De Cecco, Sandro; De Gruttola, Daniele; De Pasquale, Salvatore; De Rosa, Gianfranca; Dellacasa, G.; Derbin, Alexander; Devoto, Alberto; Di Capua, Francesco; Di Noto, L.; Di Stefano, P.; Diaz, M. Fernandez; Dolganov, G.; Dordei, Francesca; Elersich, A.; Ellingwood, E.; Erjavec, T.; Fiorillo, Giuliana; Franchini, Paolo; Franco, Davide; Funicello, Nicola; Gabriele, Federico; Gahan, D.; Galbiati, Cristiano; Gallina, Giacomo; Gallus, G.; Garbini, Marco; García Abia, Pablo; Gendotti, A.; Ghiano, Chiara; Giganti, Claudio; Giovanetti, Graham; Gola, A.; Grauso, G.; Grilli di Cortona, Giovanni; Grobov, A.; Gromov, M.; Guan, Mengyun; Guerzoni, Marco; Gulino, Marisa; Guo, C.; Hackett, B.R.; Hallin, A.L.; Hamer, A.; Haranczyk, M.; Hessel, T.; Hill, Tony; Horikawa, S.; Hubaut, Fabrice; Hucker, J.; Hugues, T.; Ianni, Andrea; Ii, F.G. Schuckman; Ippolito, Valerio; Jillings, C.; John, T. Vallivilayil; Kachru, P.; Kemp, Ashlea; Kendziora, C.L.; Kimura, M.; Kochanek, Izabela Anna; Kondo, K.; Korga, G.; Koulosousas, S.; Kubankin, A.; Kuss, Michael; Kuźniak, Marcin; La Commara, Marco; Lai, M.; Le Guirriec, Emmanuel; Leason, E.; Leoni, Alfiero; Lidey, L.; Lissia, Marcello; Luzzi, L.; Lychagina, O.; Macfadyen, Oliver; Machulin, I.N.; Manecki, S.; Manthos, Ioannis; Mapelli, L.P.; Margotti, Anselmo; Mari, Stefano Maria; Mariani, Camillo; Maricic, Jelena; Marini, Anna; Martinez, M.; Martoff, C.J.; Matteucci, Giuseppe; Mavrokoridis, Konstantinos; McDonald, Arthur; Messina, Andrea; Milincic, R.; Mitra, A.; Moharana, A.; Monroe, J.; Moretti, Elena; Morrocchi, M.; Mróz, T.; Muratova, V.N.; Muscas, C.; Musico, Paolo; Nania, Rosario; Nessi, Marzio; Nieradka, G.; Nikolopoulos, Konstantinos; Nowak, Jaroslaw; Olchansky, K.; Oleinik, A.; Oleynikov, V.; Organtini, P.; Ortiz de Solórzano, Alfonso; Pagani, L.; Pallavicini, Marco; Pandola, Luciano; Pantic, E.; Paoloni, Eugenio; Paternoster, Giovanni; Pegoraro, P.A.; Pelczar, Krzysztof; Pellegrino, Carmelo; Pesudo, V.; Piacentini, Stefano; Pietrofaccia, L.; Pino, Noemi; Pocar, A.; Poehlmann, D.M.; Pordes, Stephen; Pralavorio, Pascal; Price, Darren; Ragusa, Francesco; Ramachers, Yorck; Razeti, M.; Renshaw, Andrew; Rescigno, Marco; Retière, Fabrice; Rignanese, Luigi Pio; Ripoli, C.; Rivetti, Angelo; Roberts, A.; Roberts, C.; Rode, J.; Rogers, G.; Romero, L.; Rossi, Matteo; Rubbia, A.; Ruiz, J.M. Cela; Sabia, M.A.; Sadashivajois, Shriram; Salomone, Paolo; Sandford, Ellen; Sanfilippo, Simone; Santone, Daria; Santorelli, Roberto; Savarese, Claudio; Scapparone, Eugenio; Schillaci, Gaetano; Scioli, Gilda; Simeone, Marino; Skensved, P.; Skorokhvatov, M.D.; Smirnov, Oleg; Smirnova, T.; Smith, B.; Spadoni, F.; Spangenberg, Martin; Stefanizzi, R.; Steri, A.; Stornelli, V.; Stracka, Simone; Stringer, Katelyn; Sulis, S.; Sung, Allan; Suvorov, Y.; Szelc, Andrzej; Tartaglia, Roberto; Taylor, A.N.; Taylor, J.; Tedesco, Silvia; Testera, Gemma; Thieme, Kevin; Thorpe, Thomas; Tonazzo, Alessandra; Tricomi, Alessia Rita; Unzhakov, E.; Van Uffelen, M.; Viant, T.; Viel, Simon; Vilda, E. Conde; Vogelaar, R.B.; Vossebeld, Joost; Wada, Masayuki; Walczak, Marek; Wang, H.; Wang, Y.; Westerdale, Shawn; Williams, L. L.; Wingerter-Seez, Isabelle; Wojaczyński, R.; Wojcik, Marcin; Wright, T.; Xie, Y.; Yang, C.; Zabihi, A.; Zakhary, P.; Zani, Andrea; Zichichi, A.; Zuzel, Grzegorz; Zykova, M.P.
Source: Astropart.Phys., 152(2023), 102878, (2023-06-28)
Publisher Information: Elsevier B.V.
Publication Year: 2023
Collection: Istituto Nazionale di Fisica Nucleare (INFN): Open Access Repository
Subject Terms: Cosmogenic activation; Argon; Dark matter; Rare events; time projection chamber: liquid argon; galaxy: dark matter; copper; cosmic radiation; long-lived; background; surface; titanium; iron; direct detection; Instrumentation and Methods for Astrophysics; High Energy Physics - Experiment; Instrumentation and Detectors
Description: The activation of materials due to exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k, currently under construction at the Laboratori Nazionali del Gran Sasso, is a direct detection experiment for galactic dark matter particles, using a two-phase liquid-argon Time Projection Chamber (TPC) filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39 Ar. Despite the outstanding capability of discriminating γ/β background in argon TPCs, this background must be considered because of induced dead time or accidental coincidences mimicking dark-matter signals and it is relevant for low-threshold electron-counting measurements. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the experiment has been estimated to set requirements and procedures during preparation of the experiment and to check that it is not dominant over primordial radioactivity; particular attention has been paid to the activation of the 120 t of UAr used in DarkSide-20k. Expected exposures above ground and production rates, either measured or calculated, have been considered in detail. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. The activity of 39 Ar induced during extraction, purification and transport on surface is evaluated to be 2.8% of the activity measured in UAr by DarkSide-50 experiment, which used the same underground source, and thus considered acceptable. Other isotopes in the UAr such as 37 Ar and 3 H are shown not to be relevant due to short half-life and assumed purification methods.
Document Type: article in journal/newspaper
Language: English
Relation: https://arxiv.org/pdf/2301.12970; https://www.openaccessrepository.it/communities/inspire-hep; https://doi.org/10.1016/j.astropartphys.2023.102878; https://inspirehep.net/literature/2627835
DOI: 10.1016/j.astropartphys.2023.102878
Availability: https://doi.org/10.1016/j.astropartphys.2023.102878; https://inspirehep.net/literature/2627835
Rights: info:eu-repo/semantics/openAccess ; Creative Commons Attribution Non Commercial No Derivatives 4.0 International ; https://creativecommons.org/licenses/by-nc-nd/4.0/
Accession Number: edsbas.AA611E7
Database: BASE