RII Track-4:NSF:Measurement of charge exchange X-ray spectra using the NIST EBIT and TES microcalorimeter array

RII Track-4：NSF：使用 NIST EBIT 和 TES 微量热仪阵列测量电荷交换 X 射线光谱

• 批准号: 2132167
• 负责人: Fabian Kislat
• 金额: $ 15.92万
• 依托单位: University of New Hampshire
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-02-01 至 2025-01-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2132167&HistoricalAwards=false
• 关键词: RII; Track; NSF; Measurement; charge

A key goal of modern astronomy is to understand how the Universe works and how it evolved, eventually making life on Earth possible. Observations of X-rays emitted by stars at various stages of their life, and from the remnants of their violent deaths in supernova explosions, are a powerful tool to study the physical processes at work. The interpretation, however, of these observations relies heavily on our knowledge of the atomic physics at play. Given the expected capabilities of future observatories, the current lack of experimental data will become a limiting factor. The goal of this fellowship project is to gather experimental data about interactions of neon ions with hydrogen and helium gas commonly found in relevant astrophysical environments. These data will both improve our understanding of basic atomic physics of highly charged ions and our ability to make use of the data collected by future large space observatories. The fellowship program will also train the PI and a graduate student from the University of New Hampshire (UNH) in techniques relevant to scientific areas of national importance such as quantum sensing, quantum computing, and low-temperature physics. This will enable them to pass this knowledge on and to train graduate and undergraduate students at UNH in these fields.Charge exchange, a process in which a highly charged ion captures an electron from a neutral atom, plays a significant role in many astrophysical plasmas. It is a recombination process that results in emission line intensities that differ from collisional excitation, and can serve as an important diagnostic of the ionization balance and composition of a plasma. Correct interpretation of astrophysical data requires detailed and accurate knowledge of charge exchange cross sections, and typically relies on theoretical modeling of synthetic spectra. During two fellowship visits to the National Institute for Standards and Technology’s (NIST) Boulder Laboratories, the PI and a graduate student will carry out a sequence of measurements to test models of energy-level resolved charge exchange cross sections of highly ionized neon Ne(8,9,10)+ with neutral gasses. These benchmarks will improve the fidelity of models and our ability to interpret astrophysical X-ray data. The measurement campaign will utilize X-ray transition edge sensor microcalorimeters for high-resolution spectroscopy and a miniature Electron Beam Ion Trap to create and trap the ions. The fellowship project is intended to be the starting point of a broader collaboration between the PI and groups at NIST. It will expand beyond the PI’s current work in high-energy astrophysics enable him to participate in future measurement campaigns with highly charged ions and in the analysis of data relevant to astrophysics. Expertise gained during this fellowship will also enable the PI to carry out other X-ray measurements using equipment already available at the University of New Hampshire (UNH), and to train students at UNH in techniques relevant to scientific areas of national importance such as quantum sensing, quantum computing, and low-temperature physics.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.

现代天文学的一个关键目标是了解宇宙如何运作和如何演化，最终使地球上的生命成为可能，观测恒星在其生命的各个阶段发出的X射线，以及它们在超新星中暴力死亡的残余物。爆炸是研究工作中的物理过程的有力工具，然而，鉴于未来观测站的预期能力，对这些观测结果的解释在很大程度上依赖于我们对原子物理学的了解，目前实验数据的缺乏将成为可能。一个限制因素。该奖学金项目的目标是收集有关天体物理环境中常见的氖离子与氢和氦气相互作用的实验数据，这些数据将提高我们对高电荷离子的基本原子物理学的理解以及我们利用这些数据的能力。该奖学金计划还将利用未来大型太空天文台收集的数据，对新罕布什尔大学 (UNH) 的 PI 和一名研究生进行与国家重要科学领域相关的技术培训，例如量子传感、量子计算和低能量子计算。温度物理学。这将使他们能够传承这些知识，并培训新罕布什尔大学这些领域的研究生和本科生。电荷交换是高电荷离子从中性原子捕获电子的过程，在许多天体物理等离子体中发挥着重要作用。这是一个重组过程，会产生与碰撞激发不同的发射线强度，并且可以作为等离子体电离平衡和组成的重要诊断。天体物理数据的正确解释需要详细而准确的电荷交换交叉知识。在对美国国家标准技术研究所 (NIST) 博尔德实验室的两次访问期间，PI 和一名研究生将进行一系列测量来测试能级模型。解析了高度电离氖 Ne(8,9,10)+ 与中性气体的电荷交换截面。这些基准将提高模型的保真度以及我们解释天体物理 X 射线数据的能力。用于高分辨率光谱的 X 射线跃迁边缘传感器微热量计和用于产生和捕获离子的微型电子束离子阱。该奖学金项目旨在成为 PI 和 NIST 小组之间更广泛合作的起点。超越PI目前在高能天体物理学方面的工作，使他能够参与未来的高带电离子测量活动以及与天体物理学相关的数据分析。在该奖学金期间获得的专业知识也将使他能够参与。 PI 使用新罕布什尔大学 (UNH) 现有的设备进行其他 X 射线测量，并对 UNH 的学生进行与国家重要科学领域相关的技术培训，例如量子传感、量子计算和低该奖项反映了 NSF 的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。