Analytical considerations for optimal axion haloscope design

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The cavity haloscope provides a highly sensitive method to search for dark matter axions in the microwave regime. Experimental attempts to enhance the sensitivity have focused on improving major aspects, such as producing strong magnetic fields, increasing cavity quality factors, and achieving lowest possible noise temperatures. Minor details, however, also need to be carefully considered in realistic experimental designs. They are associated with non-uniform magnetic fields over the detection volume, noise propagation under attenuation and temperature gradients, and thermal disequilibrium in the cavity system. We take analytical approaches to these topics and offer optimal treatments for improved performance.
Publisher
IOP Publishing Ltd
Issue Date
2022-05
Language
English
Article Type
Article
Citation

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, v.49, no.5, pp.1 - 15

ISSN
0954-3899
DOI
10.1088/1361-6471/ac58b4
URI
http://hdl.handle.net/10203/296566
Appears in Collection
PH-Journal Papers(저널논문)
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