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DarkSide-20k - URANIA Project

DarkSide-20k - URANIA Project
DarkSide-20k - URANIA 项目
批准号:
1935947
负责人:
Cristiano Galbiati
金额:
$300.0万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2020
资助国家:
美国
项目状态:
未结题
起止时间:
2020-07-15 至 2025-06-30

项目摘要

项目成果

Cristiano Galbiati的其他基金

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相关文献

中文摘要
翻译
不能用可见物质来解释的引力效应是有据可查的,尽管它们的来源仍然未知。对这些观测结果的一个合理解释是,存在一种尚未被发现的基本弱相互作用大质量粒子(WIMP)。银河晕wimp相对于地球上探测器的运动可能导致wimp -核弹性碰撞,低背景,低阈值探测器能够在非常大的暴露过程中明确识别少量的核反冲。该奖项支持DarkSide-20k (DS-20k)探测器,这是一种液态氩时间投影室,旨在实现对大质量(30 GeV/c2以上)WIMP暗物质的领先灵敏度,为位于CO . Cortez的URANIA工厂提供资金,用于从地下源(UAr)中大量提取低放射性氩气。这些资金将用于由美国国家科学基金会资助的团体直接负责的基础设施。该项目的更广泛的科学影响包括发现了一种新的、商业上可行的氦源,目前占美国产量的15%,并为DS-20k生产了数百吨低放射性UAr。提取设施可以继续生产地下氩气,用于需要氩气来实现其科学目标的其他感兴趣的粒子物理实验,以及用于其他技术用途,包括禁止核试验核查和放射性测年。建造DS-20k将需要及时采购大量的UAr。这将由URANIA完成,这是一个能够每天提取250公斤氩的氩提取和净化工厂。URANIA工厂本身由意大利机构(INFN)提供资金,并将由合同供应商按照URANIA项目团队制定的规范建造。提取设施场地的准备,以及工厂的安装和调试,由nsf支持的小组负责,并由该奖项资助。这些都是项目的关键组成部分,需要美国团体的技术专长。该奖项反映了美国国家科学基金会的法定使命,并通过使用基金会的知识价值和更广泛的影响审查标准进行评估,被认为值得支持。
英文摘要
Gravitational effects that cannot be explained by visible matter are well-documented, though their source remains unknown. A well-motivated explanation for these observations is the existence of an as-yet-undiscovered elementary Weakly Interacting Massive Particle (WIMP). The motion of galactic halo WIMPs relative to a detector on Earth could result in WIMP-nucleus elastic collisions detectable by a low-background, low-threshold detector capable of unambiguously identifying a small number of nuclear recoils over the course of a very large exposure.This award supports the DarkSide-20k (DS-20k) detector, a liquid argon time projection chamber designed to achieve leading sensitivity to high-mass (above 30 GeV/c2) WIMP dark matter, by providing funding for the URANIA plant, in Cortez, CO, for the high-volume extraction of low-radioactivity argon gas from an underground source (UAr). The funds will be used for pieces of infrastructure that are the direct responsibility of the US NSF-funded groups. Scientific broader impacts of the project include the discovery of a novel, commercially viable helium source that today supplies 15% of the US production and the production of hundreds of tonnes of low-radioactivity UAr for DS-20k. The extraction facility could continue to produce underground argon for other interested particle physics experiments that require UAr to achieve their scientific objectives, as well as for other technical uses including nuclear test ban verification and radiometric dating.Constructing DS-20k will require that large amounts of UAr be procured in timely fashion. This will be accomplished by URANIA, an argon extraction and purification plant capable of extracting 250 kg/day of UAr. The URANIA plant itself is funded by the Italian Agency (INFN) and will be built by a contracted vendor following specifications established by the URANIA Project team. The preparation of the extraction facility site, as well as the installation and commissioning of the plant, falls under the responsibility of the NSF-supported groups and is funded by this award. These are the critical components of the project that require the technical expertise of the U.S. groups.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
期刊论文(24)
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科研奖励(0)
会议论文
DOI: 10.1140/epjc/s10052-023-11410-4
发表时间: 2023-02
期刊: The European Physical Journal C
影响因子: --
作者: [T. D. C. P. Agnes;I. Albuquerque;T. Alexander;A. Alton;M. Ave;H. Back;G. Batignani;K. Biery;V. Bocci;W. Bonivento;B. Bottino;S. Bussino;M. Cadeddu;M. Cadoni;F. Calaprice;A. Caminata;M. Campos;N. Canci;M. Caravati;N. Cargioli;M. Cariello;M. Carlini;V. Cataudella;P. Cavalcante;S. Cavuoti;S. Chashin;A. Chepurnov;C. Cicalò;G. Covone;D. D’Angelo;S. Davini;A. Candia;S. Cecco;G. Filippis;G. Rosa;A. Derbin;A. Devoto;M. D’Incecco;C. Dionisi;F. Dordei;M. Downing;D. D’Urso;M. Fairbairn;G. Fiorillo;D. Franco;F. Gabriele;C. Galbiati;C. Ghiano;C. Giganti;G. Giovanetti;A. Goretti;G. G. Cortona-G.;A. Grobov;M. Gromov;M. Guan;M. Gulino;B. Hackett;K. Herner;T. Hessel;B. Hosseini;F. Hubaut;E. Hungerford;A. Ianni;V. Ippolito;K. Keeter;C. Kendziora;M. Kimura;I. Kochanek;D. Korablev;G. Korga;A. Kubankin;M. Kuss;M. Commara;M. Lai;X. Li;M. Lissia;G. Longo;O. Lychagina;I. Machulin;L. Mapelli;S. Mari;J. Maricic;A. Messina;R. Milincic;J. Monroe;M. Morrocchi;X. Mougeot;V. Muratova;P. Musico;A. Nozdrina;A. Oleinik;F. Ortica;L. Pagani;M. Pallavicini;L. Pandola;E. Pantic;E. Paoloni;K. Pelczar;N. Pelliccia;S. Piacentini;A. Pocar;D. Poehlmann;S. Pordes;S. Poudel;P. Pralavorio;D. Price;F. Ragusa;M. Razeti;A. Razeto;A. Renshaw;M. Rescigno;J. Rode;A. Romani;D. Sablone;O. Samoylov;E. Sandford;W. Sands;S. Sanfilippo;C. Savarese;B. Schlitzer;D. Semenov;A. Shchagin;A. Sheshukov;M. Skorokhvatov;O. Smirnov;A. Sotnikov;S. Stracka;Y. Suvorov;R. Tartaglia;G. Testera;A. Tonazzo;E. Unzhakov;A. Vishneva;R. Vogelaar;M. Wada;H. Wang;Y. Wang;S. Westerdale;M. Wójcik;X. Xiao;C. Yang;G. Zuzel]
通讯作者: T. D. C. P. Agnes;I. Albuquerque;T. Alexander;A. Alton;M. Ave;H. Back;G. Batignani;K. Biery;V. Bocci;W. Bonivento;B. Bottino;S. Bussino;M. Cadeddu;M. Cadoni;F. Calaprice;A. Caminata;M. Campos;N. Canci;M. Caravati;N. Cargioli;M. Cariello;M. Carlini;V. Cataudella;P. Cavalcante;S. Cavuoti;S. Chashin;A. Chepurnov;C. Cicalò;G. Covone;D. D’Angelo;S. Davini;A. Candia;S. Cecco;G. Filippis;G. Rosa;A. Derbin;A. Devoto;M. D’Incecco;C. Dionisi;F. Dordei;M. Downing;D. D’Urso;M. Fairbairn;G. Fiorillo;D. Franco;F. Gabriele;C. Galbiati;C. Ghiano;C. Giganti;G. Giovanetti;A. Goretti;G. G. Cortona-G.;A. Grobov;M. Gromov;M. Guan;M. Gulino;B. Hackett;K. Herner;T. Hessel;B. Hosseini;F. Hubaut;E. Hungerford;A. Ianni;V. Ippolito;K. Keeter;C. Kendziora;M. Kimura;I. Kochanek;D. Korablev;G. Korga;A. Kubankin;M. Kuss;M. Commara;M. Lai;X. Li;M. Lissia;G. Longo;O. Lychagina;I. Machulin;L. Mapelli;S. Mari;J. Maricic;A. Messina;R. Milincic;J. Monroe;M. Morrocchi;X. Mougeot;V. Muratova;P. Musico;A. Nozdrina;A. Oleinik;F. Ortica;L. Pagani;M. Pallavicini;L. Pandola;E. Pantic;E. Paoloni;K. Pelczar;N. Pelliccia;S. Piacentini;A. Pocar;D. Poehlmann;S. Pordes;S. Poudel;P. Pralavorio;D. Price;F. Ragusa;M. Razeti;A. Razeto;A. Renshaw;M. Rescigno;J. Rode;A. Romani;D. Sablone;O. Samoylov;E. Sandford;W. Sands;S. Sanfilippo;C. Savarese;B. Schlitzer;D. Semenov;A. Shchagin;A. Sheshukov;M. Skorokhvatov;O. Smirnov;A. Sotnikov;S. Stracka;Y. Suvorov;R. Tartaglia;G. Testera;A. Tonazzo;E. Unzhakov;A. Vishneva;R. Vogelaar;M. Wada;H. Wang;Y. Wang;S. Westerdale;M. Wójcik;X. Xiao;C. Yang;G. Zuzel
Performance of the ReD TPC, a novel double-phase LAr detector with silicon photomultiplier readout
ReD TPC 的性能,一种具有硅光电倍增管读数功能的新型双相 LAr 探测器
DOI: 10.1140/epjc/s10052-021-09801-6
发表时间: 2021
期刊: The European Physical Journal C
影响因子: --
作者: [Agnes, P., Albergo, S., Albuquerque, I., Arba, M., Ave, M., Boiano, A., Bonivento, W. M., Bottino, B., Bussino, S., Cadeddu, M.]
通讯作者: Cadeddu, M.
DOI: 10.1088/1475-7516/2019/01/014
发表时间: 2017-04
期刊: Journal of Cosmology and Astroparticle Physics
影响因子: 6.4
作者: [M. Cadeddu;M. Lissia;P. Agnes;G. Batignani;W. Bonivento;B. Bottino;M. Caravati;A. Cocco;G. Covone;A. Candia;S. Catalanotti;V. Cataudella;C. Cicalò;G. Filippis;G. Rosa;S. Davini;A. Devoto;C. Dionisi;D. Franco;C. Giganti;C. Galbiati;S. Giagu;M. Gulino;M. Kuss;L. Lista;G. Longo;A. Navrer-Agasson;M. Pallavicini;L. Pandola;E. Paoloni;E. Picciau;M. Razeti;M. Rescigno;Q. Riffard;B. Rossi;N. Rossi;G. Testera;P. Trinchese;A. Tonazzo;S. Walker;G. Fiorillo]
通讯作者: M. Cadeddu;M. Lissia;P. Agnes;G. Batignani;W. Bonivento;B. Bottino;M. Caravati;A. Cocco;G. Covone;A. Candia;S. Catalanotti;V. Cataudella;C. Cicalò;G. Filippis;G. Rosa;S. Davini;A. Devoto;C. Dionisi;D. Franco;C. Giganti;C. Galbiati;S. Giagu;M. Gulino;M. Kuss;L. Lista;G. Longo;A. Navrer-Agasson;M. Pallavicini;L. Pandola;E. Paoloni;E. Picciau;M. Razeti;M. Rescigno;Q. Riffard;B. Rossi;N. Rossi;G. Testera;P. Trinchese;A. Tonazzo;S. Walker;G. Fiorillo
Parametrization of high light yield, energy resolution, and optical cross-talk in SiPM-based liquid argon detectors
基于 SiPM 的液氩探测器中高光产量、能量分辨率和光学串扰的参数化
DOI: 10.1016/j.nima.2022.167911
发表时间: 2023
期刊: Detectors and Associated Equipment
影响因子: --
作者: [Moharana, A., Galbiati, C., Horikawa, S., Kachru, P., Kochanek, I., Kondo, K., Razeto, A.]
通讯作者: Razeto, A.
21
    Collaborative Research: The DarkSide Dark-Matter Search Using Liquid Argon
    • 批准号:
      2310038
    • 项目类别:
      Continuing Grant
    • 资助金额:
      $208.99万
    • 财政年份:
      2023
    • 负责人:
      Cristiano Galbiati
    • 依托单位:
    DarkSide
    • 批准号:
      2131857
    • 项目类别:
      Cooperative Agreement
    • 资助金额:
      $1170.98万
    • 财政年份:
      2022
    • 负责人:
      Cristiano Galbiati
    • 依托单位:
    Collaborative Research: Solar Neutrino Science with Borexino
    • 批准号:
      1821080
    • 项目类别:
      Continuing Grant
    • 资助金额:
      $34.84万
    • 财政年份:
      2019
    • 负责人:
      Cristiano Galbiati
    • 依托单位:
    Collaborative Research: DarkSide-20K: A Global Program for the Direct Detection of Dark Matter Using Low-Radioactivity Argon
    • 批准号:
      1812540
    • 项目类别:
      Continuing Grant
    • 资助金额:
      $325.0万
    • 财政年份:
      2018
    • 负责人:
      Cristiano Galbiati
    • 依托单位:
    国内基金
    海外基金
    20K温区热声驱动脉冲管制冷机系统的机理研究
    • 批准号:
      50506031
    • 项目类别:
      青年科学基金项目
    • 资助金额:
      24.0万元
    • 批准年份:
      2005
    • 负责人:
      戴巍
    • 依托单位:
    20K以下温区高频脉冲管制冷机的非理想热力学过程研究
    • 批准号:
      50206025
    • 项目类别:
      青年科学基金项目
    • 资助金额:
      25.0万元
    • 批准年份:
      2002
    • 负责人:
      杨鲁伟
    • 依托单位: