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

DarkSide-20k Collaboration

doi:10.1140/epjc/s10052-021-09121-9

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

DarkSide-20k Collaboration

Research output: Contribution to journal › Article › peer-review

Original language	English
Article number	359
Journal	European Physical Journal C
Volume	81
DOIs	https://doi.org/10.1140/epjc/s10052-021-09121-9
Publication status	Published - 26 Apr 2021

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10.1140/epjc/s10052-021-09121-9Licence: CC BY

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@article{b5832dc4010049b8a4f7abe5315f5fc0,

title = "Separating 39Ar from 40Ar by cryogenic distillation with Aria for dark-matter searches",

author = "\{DarkSide-20k Collaboration\} and P. Agnes and S. Albergo and Albuquerque, \{I. F.M.\} and T. Alexander and A. Alici and Alton, \{A. K.\} and P. Amaudruz and M. Arba and P. Arpaia and S. Arcelli and M. Ave and Avetissov, \{I. Ch\} and Avetisov, \{R. I.\} and O. Azzolini and Back, \{H. O.\} and Z. Balmforth and V. Barbarian and \{Barrado Olmedo\}, A. and P. Barrillon and A. Basco and G. Batignani and A. Bondar and Bonivento, \{W. M.\} and E. Borisova and B. Bottino and Boulay, \{M. G.\} and G. Buccino and S. Bussino and J. Busto and A. Buzulutskov and M. Cadeddu and M. Cadoni and A. Caminata and Canesi, \{E. V.\} and N. Canci and G. Cappello and M. Caravati and A. Devoto and S. Hill and Kemp, \{A. A.\} and M. Leyton and X. Li and J. Mclaughlin and J. Monroe and A. Oleinik and D. Santone and B. Smith and Y. Wang and L. Williams and C. Yang",

note = "Funding Information: The second phase of the leak checks, carried out at CERN, was performed under service agreement KN3155/TE. We acknowledge the professional contribution of the Mine and Electrical Maintenance staff of Carbosulcis S.p.A. Part of the project funding comes from Intervento finanziato con risorse FSC 2014-2020 – Patto per lo Sviluppo della Regione Sardegna. This paper is based upon work supported by the U. S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004054, No. PHY-1004072, No. PHY-1242585, No. PHY-1314483, No. PHY- 1314507, associated collaborative grants, No. PHY-1211308, No. PHY-1314501, No. PHY-1455351 and No. PHY-1606912, as well as Major Research Instrumentation Grant No. MRI-1429544), the Italian Istituto Nazionale di Fisica Nucleare (Grants from Italian Ministero dell{\textquoteright}Istruzione, Universit{\`a}, e Ricerca ARIA e la Ricerca della Materia Oscura – Fondo Integrativo Speciale per la Ricerca (FISR) and Progetto Premiale 2013 and Commissione Scientifica Nazionale II). We acknowledge the financial support by LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), the Natural Sciences and Engineering Research Council of Canada, SNOLAB, Arthur B. McDonald Canadian Astroparticle Physics Research Institute, and the S{\~a}o Paulo Research Foundation (Grant No. FAPESP – 2017/26238-4). The authors were also supported by the Unidad de Excelencia Mar{\'i}a de Maeztu: CIEMAT – F{\'i}sica de part{\'i}culas (Grant No. MDM 2015-0509), the Polish National Science Centre (Grant No. UMO-2019/33/B/ST2/02884), the Foundation for Polish Science (Grant No. TEAM/2016 - 2/17), the International Research Agenda Program AstroCeNT (Grant No. MAB/2018/7) funded by the Foundation for Polish Science from the European Regional Development Fund, the European Union{\textquoteright}s Horizon 2020 research and innovation program under grant agreement No 962480, the Science and Technology Facilities Council, part of the United Kingdom Research and Innovation, and The Royal Society (United Kingdom). I.F.M.A is supported in part by Conselho Nacional de Desenvolvimento Cient{\'i}fico e Tecnol{\'o}gico (CNPq). We also wish to acknowledge the support from Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. Funding Information: The second phase of the leak checks, carried out at CERN, was performed under service agreement KN3155/TE. We acknowledge the professional contribution of the Mine and Electrical Maintenance staff of Carbosulcis S.p.A. Part of the project funding comes from Intervento finanziato con risorse FSC 2014-2020 ? Patto per lo Sviluppo della Regione Sardegna. This paper is based upon work supported by the U. S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004054, No. PHY-1004072, No. PHY-1242585, No. PHY-1314483, No. PHY- 1314507, associated collaborative grants, No. PHY-1211308, No. PHY-1314501, No. PHY-1455351 and No. PHY-1606912, as well as Major Research Instrumentation Grant No. MRI-1429544), the Italian Istituto Nazionale di Fisica Nucleare (Grants from Italian Ministero dell?Istruzione, Universit?, e Ricerca ARIA e la Ricerca della Materia Oscura ? Fondo Integrativo Speciale per la Ricerca (FISR) and Progetto Premiale 2013 and Commissione Scientifica Nazionale II). We acknowledge the financial support by LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), the Natural Sciences and Engineering Research Council of Canada, SNOLAB, Arthur B. McDonald Canadian Astroparticle Physics Research Institute, and the S?o Paulo Research Foundation (Grant No. FAPESP ? 2017/26238-4). The authors were also supported by the Unidad de Excelencia Mar?a de Maeztu: CIEMAT ? F?sica de part?culas (Grant No. MDM 2015-0509), the Polish National Science Centre (Grant No. UMO-2019/33/B/ST2/02884), the Foundation for Polish Science (Grant No. TEAM/2016 - 2/17), the International Research Agenda Program AstroCeNT (Grant No. MAB/2018/7) funded by the Foundation for Polish Science from the European Regional Development Fund, the European Union?s Horizon 2020 research and innovation program under grant agreement No 962480, the Science and Technology Facilities Council, part of the United Kingdom Research and Innovation, and The Royal Society (United Kingdom). I.F.M.A is supported in part by Conselho Nacional de Desenvolvimento Cient?fico e Tecnol?gico (CNPq). We also wish to acknowledge the support from Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. Publisher Copyright: {\textcopyright} 2021, The Author(s).",

year = "2021",

month = apr,

day = "26",

doi = "10.1140/epjc/s10052-021-09121-9",

language = "English",

volume = "81",

journal = "European Physical Journal C",

issn = "1434-6044",

publisher = "Springer New York",

}

TY - JOUR

T1 - Separating 39Ar from 40Ar by cryogenic distillation with Aria for dark-matter searches

AU - DarkSide-20k Collaboration

AU - Agnes, P.

AU - Albergo, S.

AU - Albuquerque, I. F.M.

AU - Alexander, T.

AU - Alici, A.

AU - Alton, A. K.

AU - Amaudruz, P.

AU - Arba, M.

AU - Arpaia, P.

AU - Arcelli, S.

AU - Ave, M.

AU - Avetissov, I. Ch

AU - Avetisov, R. I.

AU - Azzolini, O.

AU - Back, H. O.

AU - Balmforth, Z.

AU - Barbarian, V.

AU - Barrado Olmedo, A.

AU - Barrillon, P.

AU - Basco, A.

AU - Batignani, G.

AU - Bondar, A.

AU - Bonivento, W. M.

AU - Borisova, E.

AU - Bottino, B.

AU - Boulay, M. G.

AU - Buccino, G.

AU - Bussino, S.

AU - Busto, J.

AU - Buzulutskov, A.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Caminata, A.

AU - Canesi, E. V.

AU - Canci, N.

AU - Cappello, G.

AU - Caravati, M.

AU - Devoto, A.

AU - Hill, S.

AU - Kemp, A. A.

AU - Leyton, M.

AU - Li, X.

AU - Mclaughlin, J.

AU - Monroe, J.

AU - Oleinik, A.

AU - Santone, D.

AU - Smith, B.

AU - Wang, Y.

AU - Williams, L.

AU - Yang, C.

N1 - Funding Information: The second phase of the leak checks, carried out at CERN, was performed under service agreement KN3155/TE. We acknowledge the professional contribution of the Mine and Electrical Maintenance staff of Carbosulcis S.p.A. Part of the project funding comes from Intervento finanziato con risorse FSC 2014-2020 – Patto per lo Sviluppo della Regione Sardegna. This paper is based upon work supported by the U. S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004054, No. PHY-1004072, No. PHY-1242585, No. PHY-1314483, No. PHY- 1314507, associated collaborative grants, No. PHY-1211308, No. PHY-1314501, No. PHY-1455351 and No. PHY-1606912, as well as Major Research Instrumentation Grant No. MRI-1429544), the Italian Istituto Nazionale di Fisica Nucleare (Grants from Italian Ministero dell’Istruzione, Università, e Ricerca ARIA e la Ricerca della Materia Oscura – Fondo Integrativo Speciale per la Ricerca (FISR) and Progetto Premiale 2013 and Commissione Scientifica Nazionale II). We acknowledge the financial support by LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), the Natural Sciences and Engineering Research Council of Canada, SNOLAB, Arthur B. McDonald Canadian Astroparticle Physics Research Institute, and the São Paulo Research Foundation (Grant No. FAPESP – 2017/26238-4). The authors were also supported by the Unidad de Excelencia María de Maeztu: CIEMAT – Física de partículas (Grant No. MDM 2015-0509), the Polish National Science Centre (Grant No. UMO-2019/33/B/ST2/02884), the Foundation for Polish Science (Grant No. TEAM/2016 - 2/17), the International Research Agenda Program AstroCeNT (Grant No. MAB/2018/7) funded by the Foundation for Polish Science from the European Regional Development Fund, the European Union’s Horizon 2020 research and innovation program under grant agreement No 962480, the Science and Technology Facilities Council, part of the United Kingdom Research and Innovation, and The Royal Society (United Kingdom). I.F.M.A is supported in part by Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq). We also wish to acknowledge the support from Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. Funding Information: The second phase of the leak checks, carried out at CERN, was performed under service agreement KN3155/TE. We acknowledge the professional contribution of the Mine and Electrical Maintenance staff of Carbosulcis S.p.A. Part of the project funding comes from Intervento finanziato con risorse FSC 2014-2020 ? Patto per lo Sviluppo della Regione Sardegna. This paper is based upon work supported by the U. S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004054, No. PHY-1004072, No. PHY-1242585, No. PHY-1314483, No. PHY- 1314507, associated collaborative grants, No. PHY-1211308, No. PHY-1314501, No. PHY-1455351 and No. PHY-1606912, as well as Major Research Instrumentation Grant No. MRI-1429544), the Italian Istituto Nazionale di Fisica Nucleare (Grants from Italian Ministero dell?Istruzione, Universit?, e Ricerca ARIA e la Ricerca della Materia Oscura ? Fondo Integrativo Speciale per la Ricerca (FISR) and Progetto Premiale 2013 and Commissione Scientifica Nazionale II). We acknowledge the financial support by LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), the Natural Sciences and Engineering Research Council of Canada, SNOLAB, Arthur B. McDonald Canadian Astroparticle Physics Research Institute, and the S?o Paulo Research Foundation (Grant No. FAPESP ? 2017/26238-4). The authors were also supported by the Unidad de Excelencia Mar?a de Maeztu: CIEMAT ? F?sica de part?culas (Grant No. MDM 2015-0509), the Polish National Science Centre (Grant No. UMO-2019/33/B/ST2/02884), the Foundation for Polish Science (Grant No. TEAM/2016 - 2/17), the International Research Agenda Program AstroCeNT (Grant No. MAB/2018/7) funded by the Foundation for Polish Science from the European Regional Development Fund, the European Union?s Horizon 2020 research and innovation program under grant agreement No 962480, the Science and Technology Facilities Council, part of the United Kingdom Research and Innovation, and The Royal Society (United Kingdom). I.F.M.A is supported in part by Conselho Nacional de Desenvolvimento Cient?fico e Tecnol?gico (CNPq). We also wish to acknowledge the support from Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. Publisher Copyright: © 2021, The Author(s).

PY - 2021/4/26

Y1 - 2021/4/26

UR - https://www.scopus.com/pages/publications/85104977820

U2 - 10.1140/epjc/s10052-021-09121-9

DO - 10.1140/epjc/s10052-021-09121-9

M3 - Article

AN - SCOPUS:85104977820

SN - 1434-6044

VL - 81

JO - European Physical Journal C

JF - European Physical Journal C

M1 - 359

ER -

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

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