Developing Centimeter-scale-cavity Arrays for Axion Dark Matter Detection in the 100 Micro-electron-volt Range
Erik W. Lentz, Christian R. Boutan, Matthew S. Taubman, Kevin L. Gervais

TL;DR
This paper reports progress in developing a tunable array of centimeter-scale cavities for axion dark matter detection around 100 micro-eV, addressing frequency scaling challenges with innovative cavity array technology.
Contribution
It introduces a novel design and fabrication of a tunable cavity array for axion searches in the 100 micro-eV range, demonstrating the first such array with matched modes.
Findings
First demonstration of a tunable cavity array with axion-coupling modes in 22.88-22.93 GHz range
Successful fabrication of cm-diameter cavities using electric discharge machining
Development of mode tuning mechanisms for array optimization
Abstract
The cavity haloscope technique has been the most successful approach to date in searching for axion dark matter, owing to a confluence of factors at the GHz scale including the macroscopic size of the axion-to-photon converting cavity volume, the sophistication of present radio-frequency/microwave technologies including quantum amplifiers, and the location of the quantum limit temperature. These factors scale in a disadvantageous way overall as searches move up the axion mass/frequency scale, with the quantum limit noise temperature scaling linearly with frequency , the effective single cavity volume scaling as the inverse frequency cubed , and the axion-coupled cavity mode quality factor shrinking as for copper cavities, necessitating the search for remedies. One approach is to make up the loss in volume using an array of…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Superconducting and THz Device Technology
