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: 1719271
• 负责人: Rafael Lang
• 金额: $ 76.76万
• 依托单位: Purdue University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2017
• 资助国家: 美国
• 起止时间: 2017-09-01 至 2021-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1719271&HistoricalAwards=false
• 关键词: Collaborative; Research; Continuation; Dark; Matter

Multiple astronomical observations have established that about 85% of the matter in the universe is not made of normal atoms, but must be otherwise undetected elementary "dark matter" particles that do not emit or absorb light. Deciphering the nature of this so-called Dark Matter is of fundamental importance to cosmology, astrophysics, and high-energy particle physics. 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. Direct detection of WIMP dark matter would solve a fundamental mystery in particle physics and cosmology, providing a unique window to learning about the primary matter constituent of the Universe and of physics beyond the Standard Model of particle physics. This award supports the US groups involved in the XENON1T dark matter search program at the INFN Gran Sasso National Laboratory (LNGS) underground laboratory.The XENON project continues to captivate the imagination of the public. This is evidenced, for example, by several TV shows such as "The Big Bang Theory", which on several occasions featured XENON plots and results. Public interest in science is encouraged through talks and outreach activities. XENON1T will play a significant role in solving the dark matter puzzle, by either detecting WIMPs, or putting them under immense pressure as viable dark matter candidates. In addressing this fundamental physics problem, these awards will engage many undergraduate and graduate students as well as post-doctoral researchers, exposing them to a variety of subjects in physics and cosmology, and training them in state-of-the-art technologies, thus preparing to become future leaders in the field. Finally, 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.The program for the next four years will focus on the continued operation of the XENON1T experiment and its science data analysis. The international XENON Collaboration of 130 scientists continues to be led by the PI at Columbia University with key roles served by US members both in the management of the experiment and its scientific program. XENON1T uses the largest liquid xenon time projection chamber (TPC) built to-date, with 2 tonnes active Xe target, and the highest sensitivity to dark matter Weakly Interacting Massive Particles (WIMPs), at the level of 2 × 10^-47 cm^2 for 40 GeV WIMPs. With funding of this proposal, the US will remain in the lead of the direct search for dark matter well beyond the end of the decade.

多项天文观测已经证实，宇宙中约85%的物质不是由正常原子组成，而是必须是不发射或吸收光线的、未被探测到的原生“暗物质”粒子。破译这种所谓的暗物质的本质对宇宙学、天体物理学和高能粒子物理学具有根本的重要性。一个主要的假设是，它是由相互作用很弱的大质量粒子组成的，这些粒子是在大爆炸后不久产生的。如果WIMP是暗物质，那么它们在我们银河系中的存在可能是通过位于地下深处的探测器中原子核的散射来检测到的，以帮助排除宇宙射线的背景。直接探测WIMP暗物质将解开粒子物理学和宇宙学中的一个基本谜团，为了解宇宙的主要物质组成和超越粒子物理标准模型的物理学提供了一个独特的窗口。该奖项支持参与INFN Gran Sasso国家实验室(LNGS)地下实验室XENON1T暗物质搜索计划的美国团队。氙气项目继续吸引着公众的想象力。例如，《生活大爆炸》等几部电视剧就证明了这一点，该剧多次以氙气的情节和结果为特色。通过讲座和外展活动鼓励公众对科学的兴趣。XENON1T将在解决暗物质之谜方面发挥重要作用，它要么探测到WIMP，要么将它们作为可行的暗物质候选者置于巨大的压力之下。在解决这一基本物理问题时，这些奖项将吸引许多本科生和研究生以及博士后研究人员，让他们接触到物理学和宇宙学的各种学科，并培训他们掌握最先进的技术，从而为成为该领域的未来领导者做好准备。最后，氙气中使用的仪器和技术与广泛的应用有关，从国土安全和医学成像领域，到大数据集的分析和统计处理。未来四年的计划将专注于XENON1T实验的继续运行及其科学数据分析。130名科学家的国际氙气合作继续由哥伦比亚大学的PI领导，美国成员在实验及其科学计划的管理中发挥关键作用。XENON1T使用迄今为止建造的最大的液体氙气时间投影室(TPC)，拥有2吨活跃的Xe靶，对暗物质弱相互作用大质量粒子(WIMP)的灵敏度最高，对40GeV WIMP的水平为2×10^-47 cm^2。有了这项计划的资金，美国将在本十年结束后很长一段时间内继续在直接寻找暗物质方面处于领先地位。

项目成果

Correlated single- and few-electron backgrounds milliseconds after interactions in dual-phase liquid xenon time projection chambers

• DOI: 10.1088/1748-0221/16/07/p07014
• 发表时间: 2021-03
• 期刊: Journal of Instrumentation
• 影响因子: 1.3
• 作者: A. Kopec;Amanda L. Baxter;M. Clark;R. Lang;Shengchao Li;Juehang Qin;Riya Singh

XENON1T dark matter data analysis: Signal reconstruction, calibration, and event selection

• DOI: 10.1103/physrevd.100.052014
• 发表时间: 2019-06
• 期刊: Physical Review D
• 影响因子: 5
• 作者: E. Aprile;J. Aalbers;J. Aalbers;F. Agostini;M. Alfonsi;L. Althueser;F. Amaro;V. C. Antochi;F. Arneodo;L. Baudis;B. Bauermeister;L. Bellagamba;M. Benabderrahmane;T. Berger;P. Breur;A. Brown;E. Brown;S. Bruenner;G. Bruno;R. Budnik;C. Capelli;J. Cardoso;D. Cichon;D. Coderre;A. Colijn;J. Conrad;J. Cussonneau;M. Decowski;P. Perio;P. Gangi;A. Giovanni;S. Diglio;A. Elykov;G. Eurin;J. Fei;A. Ferella;A. Fieguth;W. Fulgione;A. G. Rosso;M. Galloway;F. Gao;M. Garbini;L. Grandi;Z. Greene;C. Hasterok;E. Hogenbirk;J. Howlett;M. Iacovacci;R. Itay;F. Joerg;S. Kazama;A. Kish;G. Koltman;A. Kopec;H. Landsman;R. Lang;L. Levinson;Q. Lin;S. Lindemann;M. Lindner;F. Lombardi;J. Lopes;E. L. Fune;C. Macolino;J. Mahlstedt;A. Manfredini;A. Manfredini;F. Marignetti;T. Undagoitia;J. Masbou;D. Masson;S. Mastroianni;M. Messina;K. Micheneau;K. Miller;A. Molinario;K. Morå;Y. Mosbacher;M. Murra;J. Naganoma;K. Ni;U. Oberlack;K. Odgers;B. Pelssers;R. Peres;R. Peres;F. Piastra;J. Pienaar;V. Pizzella;G. Plante;R. Podviianiuk;H. Qiu;D. Garc'ia;S. Reichard;B. Riedel;A. Rizzo;A. Rocchetti;N. Rupp;J. Santos;G. Sartorelli;N. Šarčević;M. Scheibelhut;S. Schindler;J. Schreiner;D. Schulte;M. Schumann;L. Lavina;M. Selvi;P. Shagin;E. Shockley;M. Silva;H. Simgen;C. Therreau;D. Thers;F. Toschi;G. Trinchero;C. Tunnell;N. Upole;M. Vargas;O. Wack;Haichen Wang;Zhou Wang;Y. Wei;C. Weinheimer;D. Wenz;C. Wittweg;J. Wulf;J. Ye;Yuan Zhang;T. Zhu;J. Zopounidis

A global analysis strategy to resolve neutrino NSI degeneracies with scattering and oscillation data

• DOI: 10.1007/jhep09(2020)106
• 发表时间: 2020-02
• 期刊: Journal of High Energy Physics
• 影响因子: 5.4
• 作者: B. Dutta;R. Lang;S. Liao;S. Sinha;L. Strigari;A. Thompson

Dark Matter Search Results from a One Ton-Year Exposure of XENON1T

• DOI: 10.1103/physrevlett.121.111302
• 发表时间: 2018-09-12
• 期刊: PHYSICAL REVIEW LETTERS
• 影响因子: 8.6
• 作者: Aprile, E.;Aalbers, J.;Zhu, T.
• 通讯作者: Zhu, T.

Intrinsic backgrounds from Rn and Kr in the XENON100 experiment

• DOI: 10.1140/epjc/s10052-018-5565-y
• 发表时间: 2018-02-16
• 期刊: EUROPEAN PHYSICAL JOURNAL C
• 影响因子: 4.4
• 作者: Aprile, E.;Aalbers, J.;Zhang, Y.
• 通讯作者: Zhang, Y.