Characterization of the HAYSTAC axion dark matter search cavity using microwave measurement and simulation techniques
Nicholas M. Rapidis, Samantha M. Lewis, Karl A. van Bibber

TL;DR
This study characterizes the HAYSTAC axion dark matter search cavity using bead perturbation and 3D electromagnetic simulations, revealing impacts of misalignments, mode crossings, and demonstrating the effectiveness of modeling for cavity optimization.
Contribution
First application of bead perturbation methods to an axion haloscope cavity, showing accurate prediction of imperfections and mode interactions through simulations.
Findings
Misalignments of 0.001 inches impact cavity performance.
Mode crossings can be benign or problematic, affecting tuning range.
Simulations closely match measurements, validating modeling approaches.
Abstract
Many searches for axion cold dark matter rely on the use of tunable electromagnetic resonators. Current detectors operate at or near microwave frequencies and use cylindrical cavities with cylindrical tuning rods. The cavity performance strongly impacts the signal power of the detector, which is expected to be very small even under optimal conditions. There is strong motivation to characterize these microwave cavities and improve their performance in order to maximize the achievable signal power. We present the results of a study characterizing the HAYSTAC (Haloscope At Yale Sensitive to Axion Cold dark matter) cavity using bead perturbation measurements and detailed 3D electromagnetic simulations. This is the first use of bead perturbation methods to characterize an axion haloscope cavity. In this study, we measured impacts of misalignments on the order of 0.001 in and demonstrated…
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