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Exploiting higher-order resonant modes for axion haloscopes · Around

2019

Exploiting higher-order resonant modes for axion haloscopes

Kim, Jinsu, Youn, SungWoo, Jeong, Junu et al.

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Understand

The haloscope is one of the most sensitive approaches to the QCD axion physics within the region where the axion is considered to be a dark matter candidate.

Current experimental sensitivities, which rely on the lowest fundamental TM010 mode of a cylindrical cavity, are limited to relatively low mass regions.
Exploiting higher-order resonant modes would be beneficial because it will enable us to extend the search range with no volume loss and higher quality factors.
This approach has been discarded mainly because of the significant degradation of form factor, and difficulty with frequency tuning.

Built on

R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Pseudoparticles
1977
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J. E. Kim, Weak-interaction singlet and strong CP invariance
1980
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A. P. Zhitnitsky, On the possible suppression of axion hadron interactions
1981
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L. F. Abbott and P. Sikivie, A cosmological bound on the invisible axion
1983
Earlier work this paper cites.
P. Sikivie, Experimental Tests of the “Invisible” Axion
1983
Earlier work this paper cites.

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Then

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2018
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2018
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J. Jeong et al
2018
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B. T. McAllister et al
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