Separating 39Ar from 40Ar by cryogenic distillation with Aria for dark-matter searches

Autor(es):Mostrar menos -

Agnes, P. ^[1] ; Albergo, S. ^{[2, 3]} ; Albuquerque, I. F. M. ^[4] ; Alexander, T. ^[5] ; Alici, A. ^{[6, 7]} ; Alton, A. K. ^[8] ; Amaudruz, P. ^[9] ; Arba, M. ^[10] ; Arpaia, P. ^[11] ; Arcelli, S. ^{[6, 7]} ; Ave, M. ^[4] ; Avetissov, I. Ch ^[12] ; Avetisov, I, R. ; Azzolini, O. ^[13] ; Back, H. O. ^[5] ; Balmforth, Z. ^[14] ; Barbarian, V ^[15] ; Barrado Olmedo, A. ^[16] ; Barrillon, P. ^[17] ; Basco, A. ^[18] ; Batignani, G. ^{[19, 20]} ; Bondar, A. ^{[21, 22]} ; Bonivento, W. M. ^[10] ; Borisova, E. ^{[21, 22]} ; Bottino, B. ^{[23, 24]} ; Boulay, M. G. ^[25] ; Buccino, G. ^[26] ; Bussino, S. ^{[27, 28]} ; Busto, J. ^[17] ; Buzulutskov, A. ^{[21, 22]} ; Cadeddu, M. ^{[10, 29]} ; Cadoni, M. ^{[10, 29]} ; Caminata, A. ^[23] ; Canesi, V, E. ; Canci, N. ^[30] ; Cappello, G. ^{[2, 3]} ; Caravati, M. ^[10] ; Cardenas-Montes, M. ^[16] ; Cargioli, N. ^{[10, 29]} ; Carlini, M. ^[31] ; Carnesecchi, F. ^{[6, 7]} ; Castello, P. ^{[10, 32]} ; Castellani, A. ^[33] ; Catalanotti, S. ^{[18, 11]} ; Cataudella, V ^{[18, 11]} ; Cavalcante, P. ^[30] ; Cavuoti, S. ^{[34, 18, 11]} ; Cebrian, S. ^[35] ; Cela Ruiz, J. M. ^[16] ; Celano, B. ^[18] ; Chashin, S. ^[15] ; Chepurnov, A. ^[15] ; Cicalo, C. ^[10] ; Cifarelli, L. ^{[6, 7]} ; Cintas, D. ^[35] ; Coccetti, F. ^{[36, 37]} ; Cocco, V ^[10] ; Colocci, M. ^{[6, 7]} ; Conde Vilda, E. ^[16] ; Consiglio, L. ^[30] ; Copello, S. ^{[23, 24]} ; Corning, J. ^[38] ; Covone, G. ^{[18, 11]} ; Czudak, P. ^[39] ; D'Aniello, M. ^[40] ; D'Auria, S. ^[41] ; Rolo, M. D. Da Rocha ^[42] ; Dadoun, O. ^[43] ; Daniel, M. ^[16] ; Davini, S. ^[23] ; De Candia, A. ^{[18, 11]} ; De Cecco, S. ^{[44, 45]} ; De Falco, A. ^{[10, 29]} ; De Filippis, G. ^{[18, 11]} ; De Gruttola, D. ^{[46, 47]} ; De Guido, G. ^[48] ; De Rosa, G. ^{[18, 11]} ; Della Valle, M. ^{[34, 18]} ; Della casa, G. ^[42] ; De Pasquale, S. ^{[46, 47]} ; Derbin, V, A. ; Devoto, A. ^{[10, 29]} ; DiNoto, L. ^[23] ; Di Eusanio, F. ^[49] ; Dionisi, C. ^{[44, 45]} ; DiStefano, P. ^[38] ; Dolganov, G. ^[50] ; Dongiovanni, D. ^[51] ; Dordei, F. ^[10] ; Downing, M. ^{[52, 53]} ; Erjavec, T. ^[54] ; Falciano, S. ^{[44, 31]} ; Farenzena, S. ^[55] ; Fernandez Diaz, M. ^[16] ; Filip, C. ^[56] ; Fiorillo, G. ^{[18, 11]} ; Franceschi, A. ^[57] ; Franco, D. ^[58] ; Frolov, E. ^{[21, 22]} ; Funicello, N. ^{[46, 47]} ; Gabriele, F. ^[30] ; Galbiati, C. ^{[31, 49, 30]} ; Garbini, M. ^{[6, 36, 37]} ; Garcia Abia, P. ^[16] ; Gendotti, A. ^[59] ; Ghiano, C. ^[30] ; Giampaolo, R. A. ^{[42, 60]} ; Giganti, C. ^[43] ; Giorgi, M. A. ^{[19, 20]} ; Giovanetti, G. K. ^[61] ; Gligan, M. L. ^[56] ; Casanueva, V. Goicoechea ^[62] ; Gola, A. ^{[63, 64]} ; Goretti, A. M. ^[30] ; Graciani Diaz, R. ^[65] ; Grigoriev, G. Y. ^[50] ; Grobov, A. ^{[66, 50]} ; Gromov, M. ^{[15, 67]} ; Guan, M. ^[68] ; Guerzoni, M. ^[6] ; Guetti, M. ^[30] ; Gulino, M. ^{[69, 70]} ; Guo, C. ^[68] ; Hackett, B. R. ^[5] ; Hallin, A. ^[71] ; Haranczyk, M. ^[39] ; Hill, S. ^[14] ; Horikawa, S. ^{[31, 30]} ; Hubaut, F. ^[17] ; Hugues, T. ^[72] ; Hungerford, V, E. ; Ianni, An ^{[49, 30]} ; Ippolito, V ^[44] ; James, C. C. ^[73] ; Jillings, C. ^{[74, 75]} ; Kachru, P. ^{[31, 30]} ; Kemp, A. A. ^[38] ; Kendziora, C. L. ^[73] ; Keppel, G. ^[13] ; Khomyakov, V, A. ; Kish, A. ^[62] ; Kochanek, I ^[30] ; Kondo, K. ^[30] ; Korga, G. ^[14] ; Kubankin, A. ^[76] ; Kugathasan, R. ^{[42, 60]} ; Kuss, M. ^[19] ; La Commara, M. ^{[18, 77]} ; La Delfa, L. ^[10] ; La Grasta, D. ^[78] ; Lai, M. ^{[10, 29, 58]} ; Lami, N. ^[55] ; Langrock, S. ^[74] ; Leyton, M. ^[18] ; Li, X. ^[49] ; Lidey, L. ^[5] ; Lippi, F. ^[55] ; Lissia, M. ^[10] ; Longo, G. ^{[18, 11]} ; Maccioni, N. ^[55] ; Machulin, I. N. ^{[66, 50]} ; Mapelli, L. ^[49] ; Marasciulli, A. ^[20] ; Margotti, A. ^[6] ; Mari, S. M. ^{[27, 28]} ; Maricic, J. ^[62] ; Marinelli, M. ^[23] ; Martinez, M. ^{[35, 79]} ; Rojas, A. D. Martinez ^{[42, 60]} ; Martini, A. ^{[55, 80]} ; Mascia, M. ^[81] ; Masetto, M. ^[78] ; Masoni, A. ^[10] ; Mazzi, A. ^{[63, 64]} ; McDonald, A. B. ^[38] ; Mclaughlin, J. ^{[9, 14]} ; Messina, A. ^{[44, 45]} ; Meyers, P. D. ^[49] ; Miletic, T. ^[62] ; Milincic, R. ^[62] ; Miola, R. ^[78] ; Moggi, A. ^[19] ; Moharana, A. ^{[31, 30]} ; Moioli, S. ^[48] ; Monroe, J. ^[14] ; Morisi, S. ^{[18, 11]} ; Morrocchi, M. ^{[19, 20]} ; Mozhevitina, E. N. ^[82] ; Mroz, T. ^[39] ; Muratova, V. N. ^[83] ; Murenu, A. ^[10] ; Muscas, C. ^{[10, 32]} ; Musenich, L. ^{[23, 24]} ; Musico, P. ^[23] ; Nania, R. ^[6] ; Napolitano, T. ^[57] ; Agasson, A. Navrer ^[43] ; Nessi, M. ^[26] ; Nikulin, I ^[76] ; Nowak, J. ^[84] ; Oleinik, A. ^[76] ; Oleynikov, V ^{[21, 22]} ; Pagani, L. ^[54] ; Pallavicini, M. ^{[23, 24]} ; Palmas, S. ^[81] ; Pandola, L. ^[69] ; Pantic, E. ^[54] ; Paoloni, E. ^{[19, 20]} ; Paternoster, G. ^{[63, 64]} ; Pegoraro, P. A. ^{[10, 32]} ; Pellegrini, L. A. ^[48] ; Pellegrino, C. ^[6] ; Pelczar, K. ^[39] ; Perotti, F. ^{[41, 33]} ; Pesudo, V ^[16] ; Picciau, E. ^{[10, 29]} ; Pietropaolo, F. ^[26] ; Pinna, T. ^[51] ; Pocar, A. ^{[52, 53]} ; Podda, P. ^[55] ; Poehlmann, D. M. ^[54] ; Pordes, S. ^[73] ; Poudel, S. S. ^[85] ; Pralavorio, P. ^[17] ; Price, D. ^[86] ; Raffaelli, F. ^[19] ; Ragusa, F. ^{[87, 41]} ; Ramirez, A. ^[85] ; Razeti, M. ^[10] ; Razeto, A. ^[30] ; Renshaw, A. L. ^[85] ; Rescia, S. ^[88] ; Rescigno, M. ^[44] ; Resnati, F. ^[26] ; Retiere, F. ^[9] ; Rignanese, L. P. ^{[6, 7]} ; Ripoli, C. ^{[46, 47]} ; Rivetti, A. ^[42] ; Rode, J. ^{[43, 58]} ; Romero, L. ^[16] ; Rossi, M. ^{[23, 24]} ; Rubbia, A. ^[59] ; Rucaj, M. ^[78] ; Sabiu, G. M. ^[55] ; Salatino, P. ^{[18, 89]} ; Samoylov, O. ^[67] ; Sanchez Garcia, E. ^[16] ; Sandford, E. ^[86] ; Sanfilippo, S. ^{[27, 28]} ; Sangiorgio, V. A. ^[48] ; Santacroce, V ^[55] ; Santone, D. ^[14] ; Santorelli, R. ^[16] ; Santucci, A. ^[51] ; Savarese, C. ^[49] ; Scapparone, E. ^[6] ; Schlitzer, B. ^[54] ; Scioli, G. ^{[6, 7]} ; Semenov, D. A. ^[83] ; Shaw, B. ^[9] ; Shchagin, A. ^[76] ; Sheshukov, A. ^[67] ; Simeone, M. ^{[18, 89]} ; Skensved, P. ^[38] ; Skorokhvatov, M. D. ^{[66, 50]} ; Smirnov, O. ^[67] ; Smith, B. ^[9] ; Sokolov, A. ^{[21, 22]} ; Stefanizzi, R. ^{[10, 29]} ; Steri, A. ^[10] ; Stracka, S. ^[19] ; Strickland, V ^[25] ; Stringer, M. ^[38] ; Sulis, S. ^{[10, 32]} ; Suvorov, Y. ^{[18, 50, 11]} ; Szelc, A. M. ^[86] ; Szucs-Balazs, J. Z. ^[56] ; Tartaglia, R. ^[30] ; Testera, G. ^[23] ; Thorpe, T. N. ^{[31, 30]} ; Tonazzo, A. ^[58] ; Torres-Lara, S. ^[85] ; Tosti, S. ^[51] ; Tricomi, A. ^{[2, 3]} ; Tuveri, M. ^[10] ; Unzhakov, V, E. ; Usai, G. ^{[10, 29]} ; John, T. Vallivilayil ^{[31, 30]} ; Vescovi, S. ^[57] ; Viant, T. ^[59] ; Viel, S. ^[25] ; Vishneva ; Vogelaar, R. B. ^[90] ; Wada, M. ^[72] ; Wang, H. ^[91] ; Wang, Y. ^[91] ; Westerdale, S. ^[10] ; Wheadon, R. J. ^[42] ; Williams, L. ^[92] ; Wojcik, Ma M. ^[39] ; Wojcik, Ma ^[93] ; Xiao, X. ^[91] ; Yang, C. ^[68] ; Zani, A. ^[26] ; Zenobio, F. ^[78] ; Zichichi, A. ^{[6, 7]} ; Zuzel, G. ^[39] ; Zykova, M. P. ^[82] ; Collaboration, DarkSide-20k

Afiliação do(s) autor(es):Mostrar menos -

^[1] Univ Houston, Dept Phys, Houston, TX 77204 - USA

^[2] Univ Catania, I-95124 Catania - Italy

^[3] INFN Catania, I-95121 Catania - Italy

^[4] Univ Sao Paulo, Inst Fis, S O Paulo 05508-090, BR-05508090 Sao Paulo - Brazil

^[5] Pacific Northwest Natl Lab, Richland, WA 99352 - USA

^[6] INFN Bologna, I-40126 Bologna - Italy

^[7] Univ Bologna, Phys Dept, I-40126 Bologna - Italy

^[8] Augustana Univ, Phys Dept, Sioux Falls, SD 57197 - USA

^[9] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3 - Canada

^[10] INFN Cagliari, I-09042 Cagliari - Italy

^[11] Univ Federico II Napoli, Phys Dept, I-80126 Naples - Italy

^[12] Mendeleev Univ Chem Technol, Moscow 125047 - Russia

^[13] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, PD - Italy

^[14] Royal Holloway Univ London, Dept Phys, Egham TW20 0EX, Surrey - England

^[15] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119234 - Russia

^[16] Ctr Invest Energet Medioambientales & Tecnol, CIEMAT, Madrid 28040 - Spain

^[17] Aix Marseille Univ, Ctr Phys Particules Marseille, CPPM, CNRS IN2P3, Marseille - France

^[18] INFN Napoli, I-80126 Naples - Italy

^[19] INFN Pisa, I-56127 Pisa - Italy

^[20] Univ Pisa, Phys Dept, I-56127 Pisa - Italy

^[21] Novosibirsk State Univ, Novosibirsk 630090 - Russia

^[22] Budker Inst Nucl Phys, Novosibirsk 630090 - Russia

^[23] INFN Genova, I-16146 Genoa - Italy

^[24] Univ Genoa, Phys Dept, I-16146 Genoa - Italy

^[25] Carleton Univ, Dept Phys, Ottawa, ON K1S 5B6 - Canada

^[26] European Org Nucl Res, CERN, CH-121123 Geneva - Switzerland

^[27] INFN Roma Tre, I-00146 Rome - Italy

^[28] Univ Roma Tre, Math & Phys Dept, I-00146 Rome - Italy

^[29] Univ Cagliari, Phys Dept, I-09042 Cagliari - Italy

^[30] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67100 Assergi, AQ - Italy

^[31] Gran Sasso Sci Inst, I-67100 Laquila - Italy

^[32] Univ Cagliari, Dept Elect & Elect Engn, I-09123 Cagliari - Italy

^[33] Politecn Milan, Civil & Environm Engn Dept, I-20133 Milan - Italy

^[34] INAF Osservatorio Astron Capodimonte, I-80131 Naples - Italy

^[35] Univ Zaragoza, Ctr Astroparticulas & Fis Altas Energias, Zaragoza 50009 - Spain

^[36] Ctr Studi & Ric Enrico Fermi, I-00184 Rome - Italy

^[37] Museo Fis, I-00184 Rome - Italy

^[38] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6 - Canada

^[39] Jagiellonian Univ, M Smoluchowski Inst Phys, PL-30348 Krakow - Poland

^[40] Univ Federico II Napoli, Dipartimento Strutture Ingn & Architettura, I-80131 Naples - Italy

^[41] INFN Milano, I-20133 Milan - Italy

^[42] INFN Torino, I-10125 Turin - Italy

^[43] Univ Paris Diderot, Sorbonne Univ, LPNHE, CNRS IN2P3, F-75252 Paris - France

^[44] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome - Italy

^[45] Sapienza Univ Roma, Phys Dept, I-00185 Rome - Italy

^[46] INFN Salerno, I-84084 Salerno - Italy

^[47] Univ Salerno, Phys Dept, I-84084 Salerno - Italy

^[48] Politecn Milan, Chem Mat & Chem Engn Dept G Natta, I-20133 Milan - Italy

^[49] Princeton Univ, Phys Dept, Princeton, NJ 08544 - USA

^[50] Natl Res Ctr, Kurchatov Inst, Moscow 123182 - Russia

^[51] ENEA, Dept Fus & Nucl Safety Technol, I-00044 Frascati - Italy

^[52] Univ Massachusetts, Amherst Ctr Fundamental Interact, Amherst, MA 01003 - USA

^[53] Univ Massachusetts, Phys Dept, Amherst, MA 01003 - USA

^[54] Univ Calif Davis, Dept Phys, Davis, CA 95616 - USA

^[55] CarboSulcis SpA Miniera Monte Sinni, I-09010 Cortoghiana - Italy

^[56] Natl Inst Res & Dev Isotope & Mol Technol, Cluj Napoca 400293 - Romania

^[57] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati - Italy

^[58] Univ Paris, CNRS, Astroparticule & Cosmol, APC, F-75013 Paris - France

^[59] Swiss Fed Inst Technol, Inst Particle Phys, CH-8093 Zurich - Switzerland

^[60] Politecn Torino, Dept Elect & Commun, I-10129 Turin - Italy

^[61] Williams Coll, Phys Dept, Williamstown, MA 01267 - USA

^[62] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 - USA

^[63] Fdn Bruno Kessler, I-38123 Povo - Italy

^[64] Trento Inst Fundamental Phys & Applicat, I-38123 Povo - Italy

^[65] Univ Barcelona, Barcelona 08028, Catalonia - Spain

^[66] Natl Res Nucl Univ MEPhI, Moscow 115409 - Russia

^[67] Dubna 141980 - Russia

^[68] Inst High Energy Phys, Beijing 100049 - Peoples R China

^[69] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95123 Catania - Italy

^[70] Univ Enna Kore, Engn & Architecture Fac, I-94100 Enna - Italy

^[71] Univ Alberta, Dept Phys, Edmonton, AB T6G 2R3 - Canada

^[72] Polish Acad Sci, AstroCeNT, Nicolaus Copernicus Astron Ctr, PL-00614 Warsaw - Poland

^[73] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA

^[74] Laurentian Univ, Dept Phys & Astron, Sudbury, ON P3E 2C6 - Canada

^[75] SNOLAB, Lively, ON P3Y 1N2 - Canada

^[76] Belgorod Natl Res Univ, Radiat Phys Lab, Belgorod 308007 - Russia

^[77] Univ Federico II Napoli, Pharm Dept, I-80131 Naples - Italy

^[78] Canesi, E., V, Polaris Srl, I-20826 Misinto - Italy

^[79] Univ Zaragoza, Fdn ARAID, Zaragoza 50009 - Spain

^[80] Minist Sviluppo Econ, I-00187 Rome - Italy

^[81] Univ Cagliari, Dept Mech Chem & Mat Engn, I-09123 Cagliari - Italy

^[82] Khomyakov, A., V, Avetisov, R., I, Mendeleev Univ Chem Technol, Moscow 125047 - Russia

^[83] Derbin, A., V, V, St Petersburg Nucl Phys Inst, Gatchina 188350 - Russia

^[84] Univ Lancaster, Phys Dept, Lancaster LA1 4YB - England

^[85] Hungerford, E., V, Univ Houston, Dept Phys, Houston, TX 77204 - USA

^[86] Univ Manchester, Dept Phys & Astron, Manchester M13 9PL, Lancs - England

^[87] Univ Milan, Phys Dept, I-20133 Milan - Italy

^[88] Brookhaven Natl Lab, Upton, NY 11973 - USA

^[89] Univ Federico II Napoli, Chem Mat & Ind Prod Engn Dept, I-80126 Naples - Italy

^[90] Virginia Tech, Blacksburg, VA 24061 - USA

^[91] Univ Calif Los Angeles, Phys & Astron Dept, Los Angeles, CA 90095 - USA

^[92] Ft Lewis Coll, Dept Phys & Engn, Durango, CO 81301 - USA

^[93] Lodz Univ Technol, Inst Appl Radiat Chem, PL-93590 Lodz - Poland

• Tipo de documento: Artigo Científico
• Fonte: EUROPEAN PHYSICAL JOURNAL C; v. 81, n. 4 APR 2021.
• Citações Web of Science: 0

Resumo

Aria is a plant hosting a 350 m cryogenic isotopic distillation column, the tallest ever built, which is being installed in a mine shaft at Carbosulcis S.p.A., Nuraxi-Figus (SU), Italy. Aria is one of the pillars of the argon dark-matter search experimental program, lead by the Global Argon Dark Matter Collaboration. It was designed to reduce the isotopic abundance of 39Ar in argon extracted from underground sources, called Underground Argon (UAr), which is used for dark-matter searches. Indeed, 39Ar is a beta -emitter of cosmogenic origin, whose activity poses background and pile-up concerns in the detectors. In this paper, we discuss the requirements, design, construction, tests, and projected performance of the plant for the isotopic cryogenic distillation of argon. We also present the successful results of the isotopic cryogenic distillation of nitrogen with a prototype plant. (AU)

• Processo FAPESP: 17/26238-4 - Deteção direta de matéria escura no experimento Darkside
• Beneficiário: Maximo David Ave Pernas
• Modalidade de apoio: Auxílio à Pesquisa - Jovens Pesquisadores