SuperCDMS SNOLAB Pre-Operations

SuperCDMS SNOLAB 预操作

基本信息

  • 批准号:
    2012936
  • 负责人:
  • 金额:
    $ 74.12万
  • 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
  • 起止时间:
    2020-09-01 至 2023-08-31
  • 项目状态:
    已结题

项目摘要

Astrophysical observations and cosmological data give strong evidence that nearly a quarter of the Universe consists of dark matter. Weakly interacting massive particles (WIMPs) and axions have been proposed as theoretically favored candidates for dark matter. This one-year award supports preliminary activities for an experiment that could address the nature of dark matter in a way that is complementary to the Large Hadron Collider, indirect detection experiments, and direct detection experiments like LZ and XENONnT that will search for WIMPs. The SuperCDMS SNOLAB Collaboration is planning a new experiment equipped with advanced cryogenic detectors that have unprecedented sensitivity to dark matter particles with masses at and below the GeV/c^2 scale. The experiment is planned to be sited in SNOLAB in Canada. The experiment’s phonon-mediated detectors have applications in cosmology, astronomy, and industry. This project will also allow the PIs to build computational skills into their existing outreach efforts through short course modules, research projects, and workshops. In addition, through these funds, the groups will leverage the SNOLAB outreach team by increasing participation in tour groups and SNOLAB on-site exhibits. The overarching outreach goal is to make a significant and equitable impact in the number of undergraduate students who pursue science careers. They propose to (1) further develop this accessible analysis environment and (2) develop short tutorials on critical data-analysis skills using the JupyterHub environment.In May 2019, the CUTE facility — a new cryogenic underground test facility located directly adjacent to the SuperCDMS SNOLAB experiment site and thus shielded from cosmic rays — was completed. The Collaboration will use this low-background testing facility to conduct a series of electronic and environmental noise characterization and mitigation campaigns, as well as systematic studies of bias voltage, charge leakage, and energy calibration to optimize detector performance and operating protocols. This work includes early testing of the electronics, DAQ, data-quality, and computing and software subsystems, exercising end-to-end readout and processing of detector data, starting with a Ge HV detector — the first test detector delivered in 2019.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.
天体物理观测和宇宙学数据提供了强有力的证据,证明宇宙的近四分之一由暗物质组成。弱相互作用大质量粒子(WIMP)和轴子被认为是理论上最受欢迎的暗物质候选者。这个为期一年的奖项支持一个实验的初步活动,该实验可以解决暗物质的性质,与大型强子对撞机,间接探测实验以及直接探测实验(如LZ和XENONNT)互补,以寻找WIMP。超级CDMS SNOLAB合作计划进行一项新的实验,配备先进的低温探测器,对质量在GeV/c^2及以下的暗物质粒子具有前所未有的灵敏度。该实验计划在加拿大的SNOLAB进行。该实验的声子介导探测器在宇宙学,天文学和工业中有应用。该项目还将使PI通过短期课程模块,研究项目和研讨会将计算技能纳入其现有的外联工作。此外,通过这些资金,这些团体将通过更多地参加旅游团和SNOLAB现场展览来利用SNOLAB外联团队。总体推广目标是在追求科学事业的本科生数量中产生重大而公平的影响。他们建议(1)进一步开发这种可访问的分析环境,(2)使用SuperCyterHub环境开发关键数据分析技能的简短教程。2019年5月,CUTE设施-一个新的低温地下测试设施-直接位于SuperCDMS SNOLAB实验场附近,因此可以屏蔽宇宙射线。该合作项目将利用这一低背景测试设施开展一系列电子和环境噪声表征和缓解活动,并对偏置电压、电荷泄漏和能量校准进行系统研究,以优化探测器性能和操作协议。这项工作包括电子、DAQ、数据质量以及计算和软件子系统的早期测试,从Ge HV探测器(2019年交付的第一个测试探测器)开始,对探测器数据进行端到端读出和处理。该奖项反映了NSF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。

项目成果

期刊论文数量(7)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
EXCESS workshop: Descriptions of rising low-energy spectra
  • DOI:
    10.21468/scipostphysproc.9.001
  • 发表时间:
    2022-02
  • 期刊:
  • 影响因子:
    5.2
  • 作者:
    P. Adari;A. Aguilar-Arevalo;D. Amidei;G. Angloher;E. Armengaud;C. Augier;L. Balogh;S. Banik;D. Baxter;C. Beaufort;G. Beaulieu;V. Belov;Y. B. Gal;G. Benato;A. Benoit;A. Bento;L. Berg'e;A. Bertolini;R. Bhattacharyya;J. Billard;I. Bloch;A. Botti;R. Breier;G. Brès;J. Bret;A. Broniatowski;A. Brossard;C. Bucci;R. Bunker;M. Cababie;M. Calvo;P. Camus;G. Cancelo;L. Canonica;F. Cappella;L. Cardani;J. Caron;N. Casali;G. Castello;A. Cazes;R. Cerulli;B. C. Vergara;D. Chaize;M. Chapellier;L. Chaplinsky;F. Charlieux;M. Chaudhuri;A. Chavarria;G. Chemin;R. Chen;H. Chen;F. Chierchie;I. Colantoni;J. Colas;J. Cooley;J.-M. Coquillat;E. Corcoran;S. Crawford;M. Crisler;A. Cruciani;P. Cushman;A. D’Addabbo;J. D'Olivo;A. Dastgheibi-Fard;M. D. J'esus;Y. Deng;J. Dent;E. Depaoli;K. Dering;S. Dharani;S. Lorenzo;A. Drlica-Wagner;L. Dumoulin;D. Durnford;B. Dutta;L. Einfalt;A. Erb;A. Erhart;R. Essig;J. Estrada;E. Etzion;O. Exshaw;F. Favela-Pérez;F. Feilitzsch;G. Moroni;N. F. Iachellini;S. Ferriol;S. Fichtinger;E. Figueroa-Feliciano;J. Filippini;D. Filosofov;J. Formaggio;M. Friedl;S. Fuard;D. Fuchs;A. Fuss;R. Gaior;A. Garai;C. Garrah;J. Gascon;G. Gerbier;M. Ghaith;V. Ghete;D. Gift;I. Giomataris;G. Giroux;A. Giuliani;P. Gorel;P. Gorla;C. Goupy;J. Goupy;C. Goy;M. Gros;P. Gros;Y. Guardincerri;C. Guerin;V. Guidi;O. Guillaudin;S. Gupta;E. Guy;P. Harrington;D. Hauff;S. Heine;S. Hertel;S. E. Holland;Z. Hong;E. Hoppe;T. Hossbach;J. Ianigro;V. Iyer;A. Jastram;M. Jevskovsk'y;Y. Jin;J. Jochum;J. Johnston;A. Juillard;D. Karaivanov;V. Kashyap;I. Katsioulas;S. Kazarcev;M. Kaznacheeva;F. Kelly;B. Kilminster;A. Kinast;L. Klinkenberg;H. Kluck;P. Knights;Y. Korn;H. Kraus;B. Krosigk;A. Kubík;N. Kurinsky;J. Lamblin;A. Langenkamper;S. Langrock;T. Lasserre;H. Lattaud;P. Lautridou;I. Lawson;S. Lee;M. Lee;A. Letessier-Selvon;D. Lhuillier;M. Li;Y.‐T. Lin;A. Lubashevskiy;R. Mahapatra;S. Maludze;M. Mancuso;I. Manthos;L. Marini;S. Marnieros;R. D. Martin;A. Matalon;J. Matthews;B. Mauri;D. Mayer;A. Mazzolari;E. Mazzucato;H. Z. Theenhausen;E. Michielin;J. Minet;N. Mirabolfathi;K. V. Mirbach;D. Misiak;P. Mitra;J. Mocellin;B. Mohanty;V. Mokina;J. Mols;A. Monfardini;F. Mounier;S. Munagavalasa;J. Muraz;X. Navick;T. Neep;H. Neog;H. Neyrial;K. Nikolopoulos;A. Nilima;C. Nones;V. Novati;P. O'Brien;L. Oberauer;E. Olivieri;M. Olmi;A. Onillon;C. Oriol;A. Orly;J. Orrell;T. Ortmann;C. Overman;C. Pagliarone;V. Paluvsov'a;P. Pari;P. Patel;L. Pattavina;F. Petricca;A. Piers;H. D. Pinckney;M. Piro;M. Platt;D. Poda;D. Ponomarev;W. Potzel;P. Povinec;F. Probst;P. Privitera;F. Pucci;K. Ramanathan;J. Réal;T. Redon;F. Reindl;R. Ren;A. Robert;J. Rocha;D. Rodrigues;R. Rogly;J. Rothe;N. Rowe;S. Rozov;I. Rozova;T. Saab;N. Saffold;T. Salagnac;J. Sander;V. Sanglard;D. Santos;Youssef Sarkis Mobarak;V. Savu;G. Savvidis;I. Savvidis;S. Schonert;K. Schaffner;N. Schermer;J. Schieck;B. Schmidt;D. Schmiedmayer;C. Schwertner;L. Scola;M. Settimo;Ye. Shevchik;V. Sibille;I. Sidelnik;A. Singal;R. Smida;M. S. Haro;T. Soldner;J. Stachurska;M. Stahlberg;L. Stefanazzi;L. Stodolsky;C. Strandhagen;R. Strauss;A. Stutz;R. Thomas;A. Thompson;J. Tiffenberg;C. Tomei;M. Traina;S. Uemura;I. Usherov;L. Vagneron;W. V. D. Pontseele;F. Fernandez;M. Vidal;M. Vignati;A. L. Virto;M. Vivier;T. Volansky;V. Wagner;F. Wagner;J. Walker;R. Ward;S. Watkins;A. Wex;M. Willers;M. Wilson;L. Winslow;E. Yakushev;T. Yu;M. Zampaolo;A. Zaytsev;V. Zema;D. Zinatulina;A. Zolotarova
  • 通讯作者:
    P. Adari;A. Aguilar-Arevalo;D. Amidei;G. Angloher;E. Armengaud;C. Augier;L. Balogh;S. Banik;D. Baxter;C. Beaufort;G. Beaulieu;V. Belov;Y. B. Gal;G. Benato;A. Benoit;A. Bento;L. Berg'e;A. Bertolini;R. Bhattacharyya;J. Billard;I. Bloch;A. Botti;R. Breier;G. Brès;J. Bret;A. Broniatowski;A. Brossard;C. Bucci;R. Bunker;M. Cababie;M. Calvo;P. Camus;G. Cancelo;L. Canonica;F. Cappella;L. Cardani;J. Caron;N. Casali;G. Castello;A. Cazes;R. Cerulli;B. C. Vergara;D. Chaize;M. Chapellier;L. Chaplinsky;F. Charlieux;M. Chaudhuri;A. Chavarria;G. Chemin;R. Chen;H. Chen;F. Chierchie;I. Colantoni;J. Colas;J. Cooley;J.-M. Coquillat;E. Corcoran;S. Crawford;M. Crisler;A. Cruciani;P. Cushman;A. D’Addabbo;J. D'Olivo;A. Dastgheibi-Fard;M. D. J'esus;Y. Deng;J. Dent;E. Depaoli;K. Dering;S. Dharani;S. Lorenzo;A. Drlica-Wagner;L. Dumoulin;D. Durnford;B. Dutta;L. Einfalt;A. Erb;A. Erhart;R. Essig;J. Estrada;E. Etzion;O. Exshaw;F. Favela-Pérez;F. Feilitzsch;G. Moroni;N. F. Iachellini;S. Ferriol;S. Fichtinger;E. Figueroa-Feliciano;J. Filippini;D. Filosofov;J. Formaggio;M. Friedl;S. Fuard;D. Fuchs;A. Fuss;R. Gaior;A. Garai;C. Garrah;J. Gascon;G. Gerbier;M. Ghaith;V. Ghete;D. Gift;I. Giomataris;G. Giroux;A. Giuliani;P. Gorel;P. Gorla;C. Goupy;J. Goupy;C. Goy;M. Gros;P. Gros;Y. Guardincerri;C. Guerin;V. Guidi;O. Guillaudin;S. Gupta;E. Guy;P. Harrington;D. Hauff;S. Heine;S. Hertel;S. E. Holland;Z. Hong;E. Hoppe;T. Hossbach;J. Ianigro;V. Iyer;A. Jastram;M. Jevskovsk'y;Y. Jin;J. Jochum;J. Johnston;A. Juillard;D. Karaivanov;V. Kashyap;I. Katsioulas;S. Kazarcev;M. Kaznacheeva;F. Kelly;B. Kilminster;A. Kinast;L. Klinkenberg;H. Kluck;P. Knights;Y. Korn;H. Kraus;B. Krosigk;A. Kubík;N. Kurinsky;J. Lamblin;A. Langenkamper;S. Langrock;T. Lasserre;H. Lattaud;P. Lautridou;I. Lawson;S. Lee;M. Lee;A. Letessier-Selvon;D. Lhuillier;M. Li;Y.‐T. Lin;A. Lubashevskiy;R. Mahapatra;S. Maludze;M. Mancuso;I. Manthos;L. Marini;S. Marnieros;R. D. Martin;A. Matalon;J. Matthews;B. Mauri;D. Mayer;A. Mazzolari;E. Mazzucato;H. Z. Theenhausen;E. Michielin;J. Minet;N. Mirabolfathi;K. V. Mirbach;D. Misiak;P. Mitra;J. Mocellin;B. Mohanty;V. Mokina;J. Mols;A. Monfardini;F. Mounier;S. Munagavalasa;J. Muraz;X. Navick;T. Neep;H. Neog;H. Neyrial;K. Nikolopoulos;A. Nilima;C. Nones;V. Novati;P. O'Brien;L. Oberauer;E. Olivieri;M. Olmi;A. Onillon;C. Oriol;A. Orly;J. Orrell;T. Ortmann;C. Overman;C. Pagliarone;V. Paluvsov'a;P. Pari;P. Patel;L. Pattavina;F. Petricca;A. Piers;H. D. Pinckney;M. Piro;M. Platt;D. Poda;D. Ponomarev;W. Potzel;P. Povinec;F. Probst;P. Privitera;F. Pucci;K. Ramanathan;J. Réal;T. Redon;F. Reindl;R. Ren;A. Robert;J. Rocha;D. Rodrigues;R. Rogly;J. Rothe;N. Rowe;S. Rozov;I. Rozova;T. Saab;N. Saffold;T. Salagnac;J. Sander;V. Sanglard;D. Santos;Youssef Sarkis Mobarak;V. Savu;G. Savvidis;I. Savvidis;S. Schonert;K. Schaffner;N. Schermer;J. Schieck;B. Schmidt;D. Schmiedmayer;C. Schwertner;L. Scola;M. Settimo;Ye. Shevchik;V. Sibille;I. Sidelnik;A. Singal;R. Smida;M. S. Haro;T. Soldner;J. Stachurska;M. Stahlberg;L. Stefanazzi;L. Stodolsky;C. Strandhagen;R. Strauss;A. Stutz;R. Thomas;A. Thompson;J. Tiffenberg;C. Tomei;M. Traina;S. Uemura;I. Usherov;L. Vagneron;W. V. D. Pontseele;F. Fernandez;M. Vidal;M. Vignati;A. L. Virto;M. Vivier;T. Volansky;V. Wagner;F. Wagner;J. Walker;R. Ward;S. Watkins;A. Wex;M. Willers;M. Wilson;L. Winslow;E. Yakushev;T. Yu;M. Zampaolo;A. Zaytsev;V. Zema;D. Zinatulina;A. Zolotarova
Investigating the sources of low-energy events in a SuperCDMS-HVeV detector
研究 SuperCDMS-HVeV 探测器中低能事件的来源
  • DOI:
    10.1103/physrevd.105.112006
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    5
  • 作者:
    Albakry, M. F.;Alkhatib, I.;Amaral, D. W. P.;Aralis, T.;Aramaki, T.;Arnquist, I. J.;Ataee Langroudy, I.;Azadbakht, E.;Banik, S.;Bathurst, C.
  • 通讯作者:
    Bathurst, C.
Ionization yield measurement in a germanium CDMSlite detector using photo-neutron sources
使用光中子源测量锗 CDMSlite 探测器中的电离产额
  • DOI:
    10.1103/physrevd.105.122002
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    5
  • 作者:
    Albakry, M. F.;Alkhatib, I.;Amaral, D. W. P.;Aralis, T.;Aramaki, T.;Arnquist, I. J.;Ataee Langroudy, I.;Azadbakht, E.;Banik, S.;Bathurst, C.
  • 通讯作者:
    Bathurst, C.
The level-1 trigger for the SuperCDMS experiment at SNOLAB
SNOLAB SuperCDMS 实验的 1 级触发器
  • DOI:
    10.1088/1748-0221/17/07/p07010
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    1.3
  • 作者:
    Wilson, J.S.;Meyer zu Theenhausen, H.;von Krosigk, B.;Azadbakht, E.;Bunker, R.;Hall, J.;Hansen, S.;Hines, B.;Loer, B.;Olsen, J.T.
  • 通讯作者:
    Olsen, J.T.
Constraints on Lightly Ionizing Particles from CDMSlite
  • DOI:
    10.1103/physrevlett.127.081802
  • 发表时间:
    2021-08-18
  • 期刊:
  • 影响因子:
    8.6
  • 作者:
    Alkhatib, I.;Amaral, D. W. P.;Zheng, L.
  • 通讯作者:
    Zheng, L.
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Jodi Cooley其他文献

Jodi Cooley的其他文献

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{{ truncateString('Jodi Cooley', 18)}}的其他基金

Collaborative Research: The SuperCDMS at SNOLAB Science Program
合作研究:SNOLAB 科学计划的 SuperCDMS
  • 批准号:
    2111457
  • 财政年份:
    2021
  • 资助金额:
    $ 74.12万
  • 项目类别:
    Continuing Grant
The SMU SuperCDMS Program
SMU SuperCDMS 计划
  • 批准号:
    2012811
  • 财政年份:
    2020
  • 资助金额:
    $ 74.12万
  • 项目类别:
    Continuing Grant
The SuperCDMS Research Program at SMU
SMU 的 SuperCDMS 研究计划
  • 批准号:
    1707704
  • 财政年份:
    2017
  • 资助金额:
    $ 74.12万
  • 项目类别:
    Continuing Grant
CAREER: Towards Second Generation Dark Matter Experiments
职业:迈向第二代暗物质实验
  • 批准号:
    1151869
  • 财政年份:
    2012
  • 资助金额:
    $ 74.12万
  • 项目类别:
    Continuing Grant

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Measurement of backgrounds with the Cryogenic Underground TEst facility and SuperCDMS SNOLAB
使用低温地下测试设施和 SuperCDMS SNOLAB 测量背景
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