为轴心暗物质实验开发超导谐振器

Thomas Braine
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引用次数: 0

摘要

轴子暗物质实验(ADMX)是首次对QCD轴子在任何质量范围内达到DFSZ灵敏度的轴子光镜搜索。QCD轴子是一种动机良好的暗物质候选体,它还解决了核物理中的强CP问题。光镜有三个必要的组成部分:一个非常强的外部磁场、一个嵌入该磁场的高 Q 值空腔谐振器和一个超灵敏的射频读出系统。本论文主要报告 ADMX 谐振器的未来发展,特别是超导射频(SRF)空腔。论文首先概述了轴子、卤镜和当前的ADMX实验,然后介绍了劳伦斯利弗莫尔国家实验室(LLNL)在SRF空腔方面所做的工作,最后介绍了ADMX "混合 "超导-铜Sidecar空腔在1D运行中的初步结果。
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Superconducting Resonator Development for the Axion Dark Matter eXperiment
The Axion Dark Matter eXperiment (ADMX) is the first axion haloscope search to reach DFSZ sensitivity in any mass range for the QCD axion. The QCD axion is a well-motivated dark matter candidate that additionally solves the strong CP problem in nuclear physics. A haloscope has three necessary components; a very strong external magnet, a high Q cavity resonator embedded in this field, and an ultra-sensitive RF read-out system. This dissertation mainly reports on the future development of the resonators for ADMX, specifically superconducting RF (SRF) cavities. It starts with an overview of axions, haloscopes, and the current ADMX experiment, followed by the work done at Lawrence Livermore National Laboratory (LLNL) on SRF cavities, and finally the preliminary results of the ADMX "hybrid" superconducting-copper Sidecar cavity in run 1D.
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