Benchmarking the design of the cryogenics system for the underground argon in DarkSide-20k
- Fond. Bruno Kessler, Trento
- Carleton U.
- GSSI, Aquila; Gran Sasso
- Warsaw, Copernicus Astron. Ctr.
- INFN, Catania; Catania U.; Catania, CSFNSM
- Sao Paulo U.
- PNL, Richland
- Wisconsin U., River Falls
- TRIUMF
- Columbia U.; Columbia U., Astron. Astrophys.
- Milan Polytechnic; INFN, Milan
- Cagliari U.; INFN, Cagliari
- Alberta U.
- Lomonosov Inst. Fine Chem. Tech.
- INFN, Legnaro
- Savannah River Labs, Aiken, S.C.
- Royal Holloway, U. of London
- Madrid, CIEMAT
- Marseille, CPPM
- Pisa U.; INFN, Pisa
- Oxford U., Theor. Phys.
- INFN, Turin; Polytech. Turin
- INFN, Rome
- INFN, Genoa; Genoa U.
- Warsaw U. of Tech.
- Rome III U.; INFN, Rome3
- INFN, Naples
- Virginia Tech.
- INFN, Genoa
- Gran Sasso
- Zaragoza U.
- SINP, Moscow
- Purdue U.; Bologna U.; INFN, Bologna
- INFN, Milan
- Laurentian U.; SNOLAB, Lively
- Gran Sasso; U. Aquila (main)
- Jagiellonian U.
- Naples U.; INFN, Naples
- INFN, Milan; Milan U.
- INFN, Turin
- INFN, Rome; Rome U.
- St. Petersburg, INP
- Queen's U., Kingston
- Princeton U.
- Kurchatov Inst., Moscow
- Belgorod State U.
- UC, Davis
- Royal Holloway, U. of London; Lancaster U.
- APC, Paris
- Liverpool U.
- Novosibirsk, IYF
- Enrico Fermi Ctr., Rome; INFN, Bologna
- Manchester U.
- Zurich, ETH
- Williams Coll.
- Hawaii U.
- Chicago U., KICP
- INFN, Bologna
- INFN, LNS; Split Tech. U.
- Beijing, Inst. High Energy Phys.
- U. Edinburgh
- Houston U.
- INFN, Pisa
- UC, Riverside
- Dubna, JINR
- Kurchatov Inst., Moscow; Moscow Phys. Eng. Inst.
- Laurentian U.; SNOLAB, Lively; Queen's U., Kingston
- Birmingham U.; Hamburg U.
- PNL, Richland; Temple U.
- Royal Holloway, U. of London; TRIUMF
- Coventry U.
- Carleton U.; GSSI, Aquila; Gran Sasso
- Lancaster U.
- Gran Sasso; Princeton U.
- INFN, LNS
- Massachusetts U., Amherst
- Birmingham U.
- Naples U.; INFN, Naples; Moscow Phys. Eng. Inst.
- Naples U.; INFN, Naples; Kurchatov Inst., Moscow
- UCLA; Los Alamos
- UCLA
- Beijing, Inst. High Energy Phys.; UCAS, Beijing
- Lewis - Clark Coll.
- Lodz, Tech. U.
- UCLA; Zhongshan U.
DarkSide-20k (DS-20k) is a dark matter detection experimentunder construction at the Laboratori Nazionali del Gran Sasso (LNGS)in Italy. It utilises ∼ 100 t of low radioactivity argon from anunderground source (UAr) in its inner detector, with half serving astarget in a dual-phase time projection chamber (TPC). The UArcryogenics system must maintain stable thermodynamic conditionsthroughout the experiment's lifetime of over10 years. Continuous removal ofimpurities and radon from the UAr is essential for maximising signalyield and mitigating background. We are developing an efficient andpowerful cryogenics system with a gas purification loop with atarget circulation rate of1000 slpm. Central to itsdesign is a condenser operated with liquid nitrogen which is pairedwith a gas heat exchanger cascade, delivering a combined coolingpower of more than 8 kW. Here wepresent the design choices in view of the DS-20k requirements, inparticular the condenser's working principle and the coolingcontrol, and we show test results obtained with a dedicatedbenchmarking platform at CERN and LNGS. We find that the thermalefficiency of the recirculation loop, defined in terms of nitrogenconsumption per argon flow rate, is95 % and the pressure in the testcryostat can be maintained within±(0.1–0.2) mbar. Wefurther detail a 5-day cool-down procedure of the test cryostat,maintaining a cooling rate typically within-2 K/h, as required for theDS-20k inner detector. Additionally, we assess the circuit's flowresistance, and the heat transfer capabilities of two heat exchangergeometries for argon phase change, used to provide gas forrecirculation. We conclude by discussing how our findings influencethe finalisation of the system design, including necessarymodifications to meet requirements and ongoing testing activities.
- Research Organization:
- APC, Paris; Alberta U.; Beijing, Inst. High Energy Phys.; Belgorod State U.; Birmingham U.; Bologna U.; Cagliari U.; Carleton U.; Catania U.; Catania, CSFNSM; Chicago U., KICP; Columbia U.; Columbia U., Astron. Astrophys.; Coventry U.; Dubna, JINR; Enrico Fermi Ctr., Rome; Fond. Bruno Kessler, Trento; GSSI, Aquila; Genoa U.; Gran Sasso; Hamburg U.; Hawaii U.; Houston U.; INFN, Bologna; INFN, Cagliari; INFN, Catania; INFN, Genoa; INFN, LNS; INFN, Legnaro; INFN, Milan; INFN, Naples; INFN, Pisa; INFN, Rome; INFN, Rome3; INFN, Turin; Jagiellonian U.; Kurchatov Inst., Moscow; Lancaster U.; Laurentian U.; Lewis - Clark Coll.; Liverpool U.; Lodz, Tech. U.; Lomonosov Inst. Fine Chem. Tech.; Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Madrid, CIEMAT; Manchester U.; Marseille, CPPM; Massachusetts U., Amherst; Milan Polytechnic; Milan U.; Moscow Phys. Eng. Inst.; Naples U.; Novosibirsk, IYF; Oxford U., Theor. Phys.; Pacific Northwest National Laboratory (PNNL), Richland, WA (United States); Pisa U.; Polytech. Turin; Princeton U.; Purdue U.; Queen's U., Kingston; Rome III U.; Rome U.; Royal Holloway, U. of London; SINP, Moscow; SNOLAB, Lively; Sao Paulo U.; Savannah River Labs, Aiken, S.C.; Split Tech. U.; St. Petersburg, INP; TRIUMF; Temple U.; U. Aquila (main); U. Edinburgh; UC, Davis; UC, Riverside; UCAS, Beijing; UCLA; Virginia Tech.; Warsaw U. of Tech.; Warsaw, Copernicus Astron. Ctr.; Williams Coll.; Wisconsin U., River Falls; Zaragoza U.; Zhongshan U.; Zurich, ETH
- Sponsoring Organization:
- US Department of Energy
- Grant/Contract Number:
- 89243024CSC000002
- OSTI ID:
- 2530135
- Report Number(s):
- FERMILAB-PUB-24-0982-V; arXiv:2408.14071; oai:inspirehep.net:2821722
- Journal Information:
- JINST, Journal Name: JINST Journal Issue: 02 Vol. 20
- Country of Publication:
- United States
- Language:
- English
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