Superconducting Resonator Development for the Axion Dark Matter eXperiment

dc.contributor.advisorRybka, Gray
dc.contributor.authorBraine, Thomas
dc.date.accessioned2024-09-09T23:14:40Z
dc.date.available2024-09-09T23:14:40Z
dc.date.issued2024-09-09
dc.date.submitted2024
dc.descriptionThesis (Ph.D.)--University of Washington, 2024
dc.description.abstractThe Axion Dark Matter eXperiment (ADMX) is the first axion haloscope search to reachDFSZ 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.
dc.embargo.termsOpen Access
dc.format.mimetypeapplication/pdf
dc.identifier.otherBraine_washington_0250E_27030.pdf
dc.identifier.urihttps://hdl.handle.net/1773/52151
dc.language.isoen_US
dc.rightsCC BY
dc.subjectPhysics
dc.subjectParticle physics
dc.subject.otherPhysics
dc.titleSuperconducting Resonator Development for the Axion Dark Matter eXperiment
dc.typeThesis

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