LZ Dark Matter Search

多项天文观测证实，宇宙中约85%的物质不是由已知粒子组成的。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。LZ是一个大约7吨重的液体氙暗物质探测器，将安装在南达科他州铅的桑福德地下研究设施(SURF)4850英尺的水平上，以寻找暗物质。这项工作将有助于该探测器的设计。与LXE相关的技术的发展将在全世界越来越多的使用稀有液体作为检测材料的实验中找到用处。这些项目还将为研究生和本科生提供辐射探测、低温和气体净化方面的技术培训。LXE在天体物理、国土安全和医学成像的伽马射线成像方面有实际应用。该探测器将使用成熟的液体氙气时间投影室技术，读出一次和二次闪烁信号用于粒子识别，并结合三维位置重建来利用液体氙气的自我屏蔽、表面伪影的去除和位置相关响应函数的校准。该设计还具有一个加载Gd的液体闪烁体否决权，该否决权将密封在中央氙气探测器周围，并提供对背景中子和伽马的强大标记。LZ实验将对WIMP暗物质具有世界领先的灵敏度，灵敏度大约是目前结果的400倍，并涵盖了大量理论上有动机的候选者。这项奖励将提供资金，使该研究小组能够继续为LZ暗物质实验做出贡献，致力于阴极高压传输系统的工作。

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. 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. LZ is a ~7-tonne liquid xenon (LXe) dark matter detector to be installed at the 4850-foot level of the Sanford Underground Research Facility (SURF) in Lead, South Dakota, to look for dark matter. This work will contribute to the design of that detector. Development of technology related to LXe will find use in the increasing number of experiments worldwide using noble liquids as detection materials. These projects will also result in technical training in radiation detection, cryogenics, and gas purification for graduate and undergraduate students. LXe has practical applications to gamma ray imaging for astrophysics, Homeland Security, and medical imaging.This detector will use established liquid xenon time projection chamber technology with readout of primary and secondary scintillation signals for particle identification, together with 3-D position reconstruction to exploit the self-shielding of the liquid xenon, removal of surface artifacts, and calibration of position-dependent response functions. The design also features a gadolinium-loaded liquid scintillator veto that will hermetically enclose the central xenon detector and provide powerful tagging of background neutrons and gammas. The LZ experiment will have world-leading sensitivity to WIMP dark matter with a sensitivity about 400 times better than current results and covering a substantial range of theoretically motivated candidates. This award will provide funding to enable this research group to continue to contribute to the LZ dark matter experiment with work on the cathode high voltage delivery system.