Accès ouvert déclaré
2023
article
Study of cosmogenic activation above ground for the DarkSide-20k experiment
A. Elersich, P. Agnes, I. Ahmad, S. Albergo, I. F. M. Albuquerque, T. Alexander, P. Amaudruz, M. Atzori Corona, M. Ave, I. Ch. Avetisov, O. Azzolini, H.O. Back, Z. Balmforth, A. Barrado-Olmedo, P. Barrillon, A. Basco, G. Batignani, V. Bocci, W. Bonivento, B. Bottino, M.G. Boulay, J. Busto, M. Cadeddu, A. Caminata, N. Canci, A. Capra, S. Caprioli, M. Caravati, N. Cargioli, P. Castello, P. Cavalcante, S. Cavuoti, S. Cebrián, J. M. Cela Ruiz, S. Chashin, A. Chepurnov, E. Chyhyrynets, L. Cifarelli, D. Cintas, M. Citterio, B. Cleveland, V. Cocco, Davide Colaiuda, E. Conde Vilda, L. Consiglio, S. Copello, G. Covone, M. Czubak, M. D’Aniello, S. D’Auria, M. Rolo, S. Davini, S. De Cecco, D. De Gruttola, S. De Pasquale, G. De Rosa, G. Dellacasa, A. Derbin, A. Devoto, F. Di Capua, L. Di Noto, P. Di Stefano, G. Dolganov, F. Dordei, E. Ellingwood, T. Erjavec, M. Fernández Díaz, G. Fiorillo, P. Franchini, D. Franco, N. Funicello, F. Gabriele, D. Gahan, C. Galbiati, G. Gallina, G. Gallus, M. Garbini, P. Garcı́a-Abia, A. Gendotti, C. Ghiano, C. Giganti, G. K. Giovanetti, V. Goicoechea Casanueva, A. Gola, G. Grauso, Giovanni Grilli di Cortona, A. Grobov, M. Gromov, M. Guan, M. Guerzoni, M. Gulino, Chunkai Guo, B.R. Hackett, A.L. Hallin, A. Hamer, M. Haranczyk, T. Hessel, Stephen Hill, S. Horikawa, F. Hubaut, J. Hucker, T. Hugues, An. Ianni, V. Ippolito, C. Jillings, S. Jois, P. Kachru, A. Kemp, C. Kendziora, Masato Kimura, I. Kochanek, K. Kondo, G. Korga, S. Koulosousas, A. Kubankin, M. Kuss, M. Kuźniak, M. La Commara, M. Laí, E. Le Guirriec, E. Leason, A. Leoni, L. Lidey, M. Lissia, L. Luzzi, O. Lychagina, O. Macfadyen, I. Machulin, I. Manthos, L. Mapelli, A. Margotti, S. M. Mari, C. Mariani, J. Maricic, A. Marini, M. Martínez, C.J. Martoff, G. Matteucci, K. Mavrokoridis, A. B. McDonald, A. Messina, Aritra Mitra, A. Moharana, J. Monroe, E. Moretti, M. Morrocchi, Tomasz Mróz, V. Muratova, Carlo Muscas, R. Nania, M. Nessi, G. Nieradka, K. Nikolopoulos, J. Nowak, K. Olchansky, A. Oleinik, V. Oleynikov, P. Organtini, A. Órtiz de Solórzano, L. Pagani, M. Pallavicini, L. Pandola, E. Paoloni, G. Paternoster, P.A. Pegoraro, K. Pelczar, C. Pellegrino, V. Pesudo, S. Piacentini, L. Pietrofaccia, N. Pino, A. Pocar, D.M. Poehlmann, S. Pordes, P. Pralavorio, D. Price, F. Ragusa, Y. Ramachers, M. Razeti, A.L. Renshaw, M. Rescigno, F. Retiere, L. P. Rignanese, C. Ripoli, A. Rivetti, A. Roberts, C. Roberts, J. Rode, G. Rogers, L. Romero, M. Rossi, A. Rubbia, M. A. Sabia, P. Salomone, S. Sanfilippo, D. Santone, R. Santorelli, C. Savarese, E. Scapparone, G. Schillaci, F. G. Schuckman, G. Scioli, M. Simeone, P. Skensved, M.D. Skorokhvatov, O. Smirnov, T. Smirnova, B. C. Smith, F. Spadoni, M. Spangenberg, A. Steri, V. Stornelli, S. Stracka, M. Stringer, Sara Sulis, A. Sung, Y. Suvorov, A. M. Szelc, R. Tartaglia, A. Taylor, J. Taylor, S. Tedesco, G. Testera, K. Thieme, T. N. Thorpe, A. Tonazzo, A. Tricomi, E. Unzhakov, T. Vallivilayil John, M. Van Uffelen, T. Viant, S. Viel, R. B. Vogelaar, J. H. Vossebeld, M. Wada, M.B. Walczak, H. Wang, Y. Wang, S. Westerdale, L. Williams, I. Wingerter-Seez, R. Wojaczyński, M. Wójcik, T. Wright, Y. Xie, Azam Zabihi, P. Zakhary, A. Zani, A. Zichichi, G. Zuzel, M. P. Zykova
8Citations signalées — pas une note de qualité
80Institutions déclarées
12Pays d’affiliation déclarés
Résumé fourni par la source
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 49.7tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. 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 120t 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 39Ar 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 37Ar and 3H are shown not to be relevant due to short half-life and assumed purification methods.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Study of cosmogenic activation above ground for the DarkSide-20k experiment
- Date Crossref
- 01/10/2023
- Éditeur
- Elsevier BV
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.
Institutions déclarées
University of CataniaIstituto Nazionale di Fisica Nucleare, Sezione di CataniaUniversity of California, DavisGran Sasso Science InstituteNicolaus Copernicus Astronomical CenterPolish Academy of SciencesUniversidade de São PauloPacific Northwest National LaboratoryAugustana UniversityTRIUMFD. Mendeleyev University of Chemical Technology of RussiaIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali di LegnaroRoyal Holloway University of LondonCentro de Investigaciones Energéticas, Medioambientales y TecnológicasCentre National de la Recherche ScientifiqueCentre de physique des particules de MarseilleInstitut National de Physique Nucléaire et de Physique des ParticulesIstituto Nazionale di Fisica Nucleare, Sezione di NapoliUniversity of PisaIstituto Nazionale di Fisica Nucleare, Sezione di PisaIstituto Nazionale di Fisica Nucleare, Sezione di Roma ICarleton UniversityUniversity of CagliariIstituto Nazionale di Fisica Nucleare, Sezione di GenovaLomonosov Moscow State UniversityUniversity of Naples Federico IIUniversity of GenoaPrinceton UniversityUniversité Paris CitéLaboratoire AstroParticule et CosmologieSorbonne UniversitéIstituto Nazionale di Fisica Nucleare, Sezione di TorinoLaboratoire de Physique Nucléaire et de Hautes ÉnergiesNational Research Nuclear University MEPhIIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoUniversity of BolognaIstituto Nazionale di Fisica Nucleare, Sezione di BolognaQueen's UniversityIstituto Nazionale di Fisica Nucleare, Sezione di MilanoMoscow State UniversitySnolabLaurentian UniversityUniversity of L'AquilaTorino e-districtJagiellonian UniversityRoma Tre UniversityVirginia TechFundacion Agencia Aragonesa para la Investigacion y el DesarrolloTemple UniversityUniversity of LiverpoolSapienza University of RomeUniversity of SalernoUniversity of WarwickPetersburg Nuclear Physics InstituteLancaster UniversityKurchatov InstituteNovosibirsk State UniversityBudker Institute of Nuclear PhysicsUniversidad de ZaragozaETH ZurichFondazione Bruno KesslerAmherst CollegeUniversity of Massachusetts AmherstWilliams CollegeUniversity of ManchesterUniversity of MilanUniversity of HoustonIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsUniversity of EdinburghJoint Institute for Nuclear ResearchInstitute for Nuclear ResearchInstitute of High Energy PhysicsUniversità degli Studi di Enna KorePolitecnico di TorinoUniversity of California, Los AngelesUniversity of Chinese Academy of SciencesUniversity of California, RiversideFort Lewis CollegeInstitute of PhysicsUniversity of Birmingham Une affiliation ne permet pas de déduire la nationalité d’un auteur.
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