Collaborative Research: Continuation of the XENON Dark Matter Search at LNGS

合作研究:在 LNGS 继续进行氙暗物质搜索

基本信息

  • 批准号:
    1413358
  • 负责人:
  • 金额:
    $ 62.1万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2014
  • 资助国家:
    美国
  • 起止时间:
    2014-09-01 至 2017-08-31
  • 项目状态:
    已结题

项目摘要

Multiple astronomical observations have established that about 85% of the matter in the universe is not made of known particles. Deciphering the nature of this so-called Dark Matter is of fundamental importance to cosmology, astrophysics, and high-energy particle physics with profound implications for our view of the Universe. A leading hypothesis is that it is comprised of Weakly Interacting Massive Particles, or WIMPs, that were produced moments after the Big Bang. If WIMPs are the dark matter, then their presence in our galaxy may be detectable via scattering from atomic nuclei in detectors located deep underground to help reject backgrounds due to cosmic rays.The identification of Dark Matter (DM) poses a challenge that is being addressed with a variety of complementary approaches and technologies. The direct search for DM with the XENON project at the Gran Sasso laboratory promises an extremely cost-efficient approach to cover vast regions of expected DM parameter space. This award will enable the US groups in XENON to participate in the operations and data analysis of XENON100 well into 2015 when the start of the scientific program with XENON1T is expected. With a strong presence at Gran Sasso, the US groups will maintain a leading role in the commissioning and operation of XENON1T. Broader Impacts:A number of students as well as post-doctoral researchers are involved in the XENON project at universities across the US. They are exposed to a variety of subjects in fundamental physics and cosmology, and trained in the development and application of state-of-the-art technologies, preparing them to become future leaders in the field. The instrumentation and techniques used in XENON are relevant to a wide range of applications, from areas in homeland security and medical imaging, to the analysis and statistical treatment of large data sets.
多次天文观察结果表明,宇宙中约有85%的物质不是由已知粒子制成的。破译这种所谓的暗物质的性质对于宇宙学,天体物理学和高能量粒子物理学至关重要,对我们对宇宙的看法具有深远的影响。一个主要的假设是,它由弱相互作用的巨大颗粒或wimps组成,这些颗粒或wimps是在大爆炸后瞬间产生的。如果wimps是暗物质,那么它们在我们的星系中的存在可能可以通过在地下深处的探测器中散射从原子核中散射来检测到它们,以帮助拒绝由于宇宙射线而引起的背景。暗物质(DM)构成了一个挑战,该挑战正在通过各种互补的方法和技术来解决。 Gran Sasso实验室的XENON项目的直接搜索DM承诺采用极其成本效益的方法来涵盖庞大的预期DM参数空间。该奖项将使XENON的美国团体能够在2015年的Xenon100进行操作和数据分析,直到有望通过Xenon1t的科学计划开始。在格兰·萨索(Gran Sasso)的强大存在下,美国团体将在Xenon1t的调试和运作中保持领导作用。更广泛的影响:许多学生和博士后研究人员都参与了美国大学的Xenon项目。他们接触了基本物理和宇宙学领域的各种科目,并接受了最先进技术的开发和应用培训,这使他们成为该领域的未来领导者。 XENON中使用的仪器和技术与广泛的应用相关,从国土安全和医学成像的领域到大型数据集的分析和统计处理。

项目成果

期刊论文数量(1)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Signal yields of keV electronic recoils and their discrimination from nuclear recoils in liquid xenon
  • DOI:
    10.1103/physrevd.97.092007
  • 发表时间:
    2017-09
  • 期刊:
  • 影响因子:
    5
  • 作者:
    E. Aprile;J. Aalbers;F. Agostini;M. Alfonsi;F. Amaro;M. Anthony;F. Arneodo;P. Barrow;L. Baudis;B. Bauermeister;M. Benabderrahmane;T. Berger;P. Breur;A. Brown;E. Brown;S. Bruenner;G. Bruno;R. Budnik;L. Butikofer;J. Calvén;J. Cardoso;M. Cervantes;D. Cichon;D. Coderre;A. Colijn;J. Conrad;J. Cussonneau;M. P. Decowski;P. Perio;P. Gangi;A. Giovanni;S. Diglio;G. Eurin;J. Fei;A. Ferella;A. Fieguth;W. Fulgione;A. G. Rosso;M. Galloway;F. Gao;M. Garbini;C. Geis;L. Goetzke;L. Grandi;Z. Greene;C. Grignon;C. Hasterok;E. Hogenbirk;R. Itay;B. Kaminsky;S. Kazama;G. Kessler;A. Kish;H. Landsman;R. Lang;D. Lellouch;L. Levinson;Q. Lin;S. Lindemann;M. Lindner;F. Lombardi;J. Lopes;A. Manfredini;I. Mariş;T. Undagoitia;J. Masbou;F. V. Massoli;D. Masson;D. Mayani;M. Messina;K. Micheneau;A. Molinario;K. Moraa;M. Murra;J. Naganoma;K. Ni;U. Oberlack;P. Pakarha;B. Pelssers;R. Persiani;F. Piastra;J. Pienaar;V. Pizzella;M. Piro;G. Plante;N. Priel;D. R. Garc'ia;L. Rauch;S. Reichard;C. Reuter;A. Rizzo;N. Rupp;R. Saldanha;J. M. F. Santos;G. Sartorelli;M. Scheibelhut;S. Schindler;J. Schreiner;M. Schumann;L. Lavina;M. Selvi;P. Shagin;E. Shockley;M. Silva;H. Simgen;M. Sivers;A. Stein;D. Thers;A. Tiseni;G. Trinchero;C. Tunnell;M. Vargas;H. Wang;Z. Wang;Y. Wei;C. Weinheimer;J. Wulf;J. Ye;Y. Zhang
  • 通讯作者:
    E. Aprile;J. Aalbers;F. Agostini;M. Alfonsi;F. Amaro;M. Anthony;F. Arneodo;P. Barrow;L. Baudis;B. Bauermeister;M. Benabderrahmane;T. Berger;P. Breur;A. Brown;E. Brown;S. Bruenner;G. Bruno;R. Budnik;L. Butikofer;J. Calvén;J. Cardoso;M. Cervantes;D. Cichon;D. Coderre;A. Colijn;J. Conrad;J. Cussonneau;M. P. Decowski;P. Perio;P. Gangi;A. Giovanni;S. Diglio;G. Eurin;J. Fei;A. Ferella;A. Fieguth;W. Fulgione;A. G. Rosso;M. Galloway;F. Gao;M. Garbini;C. Geis;L. Goetzke;L. Grandi;Z. Greene;C. Grignon;C. Hasterok;E. Hogenbirk;R. Itay;B. Kaminsky;S. Kazama;G. Kessler;A. Kish;H. Landsman;R. Lang;D. Lellouch;L. Levinson;Q. Lin;S. Lindemann;M. Lindner;F. Lombardi;J. Lopes;A. Manfredini;I. Mariş;T. Undagoitia;J. Masbou;F. V. Massoli;D. Masson;D. Mayani;M. Messina;K. Micheneau;A. Molinario;K. Moraa;M. Murra;J. Naganoma;K. Ni;U. Oberlack;P. Pakarha;B. Pelssers;R. Persiani;F. Piastra;J. Pienaar;V. Pizzella;M. Piro;G. Plante;N. Priel;D. R. Garc'ia;L. Rauch;S. Reichard;C. Reuter;A. Rizzo;N. Rupp;R. Saldanha;J. M. F. Santos;G. Sartorelli;M. Scheibelhut;S. Schindler;J. Schreiner;M. Schumann;L. Lavina;M. Selvi;P. Shagin;E. Shockley;M. Silva;H. Simgen;M. Sivers;A. Stein;D. Thers;A. Tiseni;G. Trinchero;C. Tunnell;M. Vargas;H. Wang;Z. Wang;Y. Wei;C. Weinheimer;J. Wulf;J. Ye;Y. Zhang
共 1 条
  • 1
前往

Hanguo Wang其他文献

Borexino: geo-neutrino measurement at Gran Sasso, Italy
Borexino:意大利格兰萨索的地中微子测量
  • DOI:
    10.4401/ag-7389
    10.4401/ag-7389
  • 发表时间:
    2017
    2017
  • 期刊:
  • 影响因子:
    1
  • 作者:
    M. Agostini;K. Altenmüller;S. Appel;G. Bellini;J. Benziger;D. Bick;G. Bonfini;D. Bravo;B. Caccianiga;F. Calaprice;A. Caminata;P. Cavalcante;A. Chepurnov;D. D’Angelo;S. Davini;A. Derbin;L. Noto;I. Drachnev;A. Etenko;K. Fomenko;A. Formozov;D. Franco;F. Gabriele;C. Galbiati;C. Ghiano;M. Giammarchi;M. Goeger;A. Goretti;M. Gromov;C. Hagner;E. Hungerford;A. Ianni;A. Ianni;K. Jędrzejczak;D. Jeschke;V. Kobychev;D. Korablev;G. Korga;D. Kryn;M. Laubenstein;B. Lehnert;E. Litvinovich;F. Lombardi;P. Lombardi;L. Ludhova;G. Lukyanchenko;I. Machulin;S. Manecki;W. Maneschg;S. Marcocci;E. Meroni;M. Meyer;L. Miramonti;M. Misiaszek;M. Montuschi;P. Mosteiro;V. Muratova;B. Neumair;L. Oberauer;M. Obolensky;F. Ortica;M. Pallavicini;L. Papp;L. Perasso;A. Pocar;G. Ranucci;A. Razeto;A. Re;A. Romani;R. Roncin;N. Rossi;S. Schönert;D. Semenov;H. Simgen;M. Skorokhvatov;O. Smirnov;A. Sotnikov;S. Sukhotin;Y. Suvorov;R. Tartaglia;G. Testera;J. Thurn;Maria Toropova;E. Unzhakov;A. Vishneva;R. Vogelaar;F. Feilitzsch;Hanguo Wang;S. Weinz;J. Winter;M. Wójcik;M. Wurm;Z. Yokley;O. Zaimidoroga;S. Zavatarelli;K. Zuber;G. Zuzel
    M. Agostini;K. Altenmüller;S. Appel;G. Bellini;J. Benziger;D. Bick;G. Bonfini;D. Bravo;B. Caccianiga;F. Calaprice;A. Caminata;P. Cavalcante;A. Chepurnov;D. D’Angelo;S. Davini;A. Derbin;L. Noto;I. Drachnev;A. Etenko;K. Fomenko;A. Formozov;D. Franco;F. Gabriele;C. Galbiati;C. Ghiano;M. Giammarchi;M. Goeger;A. Goretti;M. Gromov;C. Hagner;E. Hungerford;A. Ianni;A. Ianni;K. Jędrzejczak;D. Jeschke;V. Kobychev;D. Korablev;G. Korga;D. Kryn;M. Laubenstein;B. Lehnert;E. Litvinovich;F. Lombardi;P. Lombardi;L. Ludhova;G. Lukyanchenko;I. Machulin;S. Manecki;W. Maneschg;S. Marcocci;E. Meroni;M. Meyer;L. Miramonti;M. Misiaszek;M. Montuschi;P. Mosteiro;V. Muratova;B. Neumair;L. Oberauer;M. Obolensky;F. Ortica;M. Pallavicini;L. Papp;L. Perasso;A. Pocar;G. Ranucci;A. Razeto;A. Re;A. Romani;R. Roncin;N. Rossi;S. Schönert;D. Semenov;H. Simgen;M. Skorokhvatov;O. Smirnov;A. Sotnikov;S. Sukhotin;Y. Suvorov;R. Tartaglia;G. Testera;J. Thurn;Maria Toropova;E. Unzhakov;A. Vishneva;R. Vogelaar;F. Feilitzsch;Hanguo Wang;S. Weinz;J. Winter;M. Wójcik;M. Wurm;Z. Yokley;O. Zaimidoroga;S. Zavatarelli;K. Zuber;G. Zuzel
  • 通讯作者:
    G. Zuzel
    G. Zuzel
Xenon as a detector for dark matter search
氙作为暗物质搜索探测器
  • DOI:
  • 发表时间:
    1998
    1998
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Hanguo Wang
    Hanguo Wang
  • 通讯作者:
    Hanguo Wang
    Hanguo Wang
WIMP Detection Using Liquid Xenon
使用液氙检测 WIMP
  • DOI:
  • 发表时间:
    1998
    1998
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Hanguo Wang
    Hanguo Wang
  • 通讯作者:
    Hanguo Wang
    Hanguo Wang
Using xenon-doped liquid argon scintillation for total-body, TOF-PET
使用掺氙液氩闪烁进行全身 TOF-PET
  • DOI:
  • 发表时间:
    2024
    2024
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Alejandro Ramirez;A. Zabihi;Xinran Li;Michela Lai;Iftikhar Ahmad;Masayuki Wada;Andrew Renshaw;Davide Franco;Hanguo Wang;F. Gabriele;C. Galbiati
    Alejandro Ramirez;A. Zabihi;Xinran Li;Michela Lai;Iftikhar Ahmad;Masayuki Wada;Andrew Renshaw;Davide Franco;Hanguo Wang;F. Gabriele;C. Galbiati
  • 通讯作者:
    C. Galbiati
    C. Galbiati
共 4 条
  • 1
前往

Hanguo Wang的其他基金

Collaborative Research: DarkSide-20k
合作研究:DarkSide-20k
  • 批准号:
    1622337
    1622337
  • 财政年份:
    2018
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Collaborative Research: DarkSide-20k: A Global Program for the Direct Detection of Dark Matter Using Low-Radioactivity Argon
合作研究:DarkSide-20k:使用低放射性氩直接探测暗物质的全球计划
  • 批准号:
    1812547
    1812547
  • 财政年份:
    2018
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Collaborative Research: Continuation of the Dark Matter Search with XENON1T at LNGS
合作研究:在 LNGS 上使用 XENON1T 继续暗物质搜索
  • 批准号:
    1719268
    1719268
  • 财政年份:
    2017
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Standard Grant
    Standard Grant
Collaborative Research: Direct Search for Dark Matter with Underground Argon at LNGS
合作研究:在 LNGS 中用地下氩直接寻找暗物质
  • 批准号:
    1314501
    1314501
  • 财政年份:
    2014
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Collaborative Research: R & D Toward DarkSide-G2, a Second-Generation Direct Search for Dark Matter
合作研究:R
  • 批准号:
    1242545
    1242545
  • 财政年份:
    2012
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Standard Grant
    Standard Grant
Collaborative Research: Continuation of the XENON100 Dark Matter Search at the Gran Sasso Underground Laboratory
合作研究:格兰萨索地下实验室继续进行 XENON100 暗物质搜索
  • 批准号:
    1104720
    1104720
  • 财政年份:
    2011
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Collaborative Research: A Depleted Argon Detector for a Dark Matter Search
合作研究:用于暗物质搜索的贫氩探测器
  • 批准号:
    1004060
    1004060
  • 财政年份:
    2010
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Collaborative Proposal: Continuation of th XENON Dark Matter Project: Construction and Underground Operation of an Upgraded XENON100 Detector
合作提案:XENON 暗物质项目的延续:升级版 XENON100 探测器的建造和地下运行
  • 批准号:
    0904224
    0904224
  • 财政年份:
    2009
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Standard Grant
    Standard Grant
DUSEL R&D: New WIMP Detector Technique Based on High Pressure Xenon Gas
杜塞尔R
  • 批准号:
    0810283
    0810283
  • 财政年份:
    2008
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Standard Grant
    Standard Grant
Request for continued operation and study of the ZEPLIN II dark matter detector
请求继续运行和研究 ZEPLIN II 暗物质探测器
  • 批准号:
    0653459
    0653459
  • 财政年份:
    2007
  • 资助金额:
    $ 62.1万
    $ 62.1万
  • 项目类别:
    Continuing Grant
    Continuing Grant

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  • 批准号:
    10704577
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Collaborative Research: NSF-BSF: Continuation of the XENON Program at LNGS
合作研究:NSF-BSF:LNGS 氙气项目的延续
  • 批准号:
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  • 批准号:
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