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High-frequency microwave cavity design for high-mass dark matter axion searches |
| Chi Zhang(张驰)1,2, Jia Wang(王佳)1, Chunguang Li(李春光)1, Shiguang Chen(陈石广)1,2, Hang Cheng(程航)1,2, Liang Sun(孙亮)1,3, and Yun Wu(吴云)1,2,4,† |
1 Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China;
2 University of Chinese Academy of Sciences, Beijing 100049, China;
3 Songshan Lake Materials Laboratory, Dongguan 523808, China;
4 Hefei National Laboratory, Hefei 230088, China |
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Abstract The haloscope based on the $\rm TM_{010}$ mode cavity is a well-established technique for detecting QCD axions. However, the method has limitations in detecting high-mass axion due to significant volume loss in the high-frequency cavity. Utilizing a higher-order mode cavity can effectively reduce the volume loss of the high-frequency cavity. The rotatable dielectric pieces as a tuning mechanism can compensate for the degradation of the form factor of the higher-order mode. Nevertheless, the introduction of dielectric causes additional volume loss. To address these issues, this paper proposes a novel design scheme by adding a central metal rod to the higher-order mode cavity tuned by dielectrics, which improves the performance of the haloscope due to the increased effective volume of the cavity detector. The superiority of the novel design is demonstrated by comparing its simulated performance with previous designs. Moreover, the feasibility of the scheme is verified by the full-wave simulation results of the mechanical design model.
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Received: 01 February 2024
Revised: 14 March 2024
Accepted manuscript online: 18 March 2024
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PACS:
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42.60.Da
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(Resonators, cavities, amplifiers, arrays, and rings)
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95.35.+d
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(Dark matter)
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| Fund: Project supported in part by the Equipment Development Project for Scientific Research of the Chinese Academy of Sciences (Grant No. YJKYYQ20190049), the Innovation Program for Quantum Science and Technology (Grant No. 2021ZD0301800), and the National Key R&D Program of China (Grant No. 2022YFA1603904). |
Corresponding Authors:
Yun Wu
E-mail: wuyun@iphy.ac.cn
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Cite this article:
Chi Zhang(张驰), Jia Wang(王佳), Chunguang Li(李春光), Shiguang Chen(陈石广), Hang Cheng(程航), Liang Sun(孙亮), and Yun Wu(吴云) High-frequency microwave cavity design for high-mass dark matter axion searches 2024 Chin. Phys. B 33 054211
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[1] Stecker F W and Shafi Q 1983 Phys. Rev. Lett. 50 928
[2] Sikivie P 1983 Phys. Rev. Lett. 51 1415
[3] Sikivie P 1985 Phys. Rev. D 32 2988
[4] Hagmann C, Sikivie P, Sullivan N, Tanner D B and Cho S I 2015 Rev. Sci. Instrum. 61 1076
[5] Asztalos S J, Carosi G, Hagmann C, Kinion D, Van Bibber K, Hotz M, Rosenberg L J, Rybka G, Hoskins J, Hwang J, Sikivie P, Tanner D B, Bradley R and Clarke J 2010 Phys. Rev. Lett. 104 041301
[6] Braine T, Cervantes R, Crisosto N, Du N, Kimes S, Rosenberg L J, Rybka G, Yang J, Bowring D, Chou A S, Khatiwada R, Sonnenschein A, Wester W, Carosi G, Woollett N, Duffy L D, Bradley R, Boutan C, Jones M, LaRoque B H, Oblath N S, Taubman M S, Clarke J, Dove A, Eddins A, O’Kelley S R, Nawaz S, Siddiqi I, Stevenson N, Agrawal A, Dixit A V, Gleason J R, Jois S, Sikivie P, Solomon J A, Sullivan N S, Tanner D B, Lentz E, Daw E J, Buckley J H, Harrington P M, Henriksen E A and Murch K W 2020 Phys. Rev. Lett. 124 101303
[7] Hoskins J, Hwang J, Martin C, Sikivie P, Sullivan N S, Tanner D B, Hotz M, Rosenberg L J, Rybka G, Wagner A, Asztalos S J, Carosi G, Hagmann C, Kinion D, Van Bibber K, Bradley R and Clarke J 2011 Phys. Rev. D 84 121302
[8] Khatiwada R, Bowring D, Chou A S, Sonnenschein A, Wester W, Mitchell D V, Braine T, Bartram C, Cervantes R, Crisosto N, Du N, Rosenberg L J, Rybka G, Yang J, Will D, Kimes S, Carosi G, Woollett N, Durham S, Duffy L D, Bradley R, Boutan C, Jones M, Laroque B H, Oblath N S, Taubman M S, Tedeschi J, Clarke J, Dove A, Hashim A, Siddiqi I, Stevenson N, Eddins A, O’Kelley S R, Nawaz S, Agrawal A, Dixit A V, Gleason J R, Jois S, Sikivie P, Sullivan N S, Tanner D B, Solomon J A, Lentz E, Daw E J, Perry M G, Buckley J H, Harrington P M, Henriksen E A, Murch K W and Hilton G C 2021 Rev. Sci. Instrum. 92 124502
[9] Buschmann M, Foster J W and Safdi B R 2020 Phys. Rev. Lett. 124 161103
[10] Klaer V B and Moore G D 2017 J. Cosmol. Astropart. Phys. 2017 049
[11] Rapidis N M, Lewis S M and van Bibber K A 2019 Rev. Sci. Instrum. 90 024706
[12] Kuo C L 2020 J. Cosmol. Astropart. Phys. 2020 010
[13] Stern I, Chisholm A A, Hoskins J, Sikivie P, Sullivan N S, Tanner D B, Carosi G and van Bibber K 2015 Rev. Sci. Instrum. 86 123305
[14] Jeong J, Youn S, Ahn S, Kim J E and Semertzidis Y K 2018 Phys. Lett. B 777 412
[15] Kim J, Youn S, Jeong J, Chung W, Kwon O and Semertzidis Y K 2020 J. Phys. G: Nucl. Part. Phys. 47 035203
[16] Read J I 2014 J. Phys. G: Nucl. Part. Phys. 41 063101
[17] Alesini D, Braggio C, Carugno G, Crescini N, D’Agostino D, Di Gioacchino D, Di Vora R, Falferi P, Gambardella U, Gatti C, Iannone G, Ligi C, Lombardi A, Maccarrone G, Ortolan A, Pengo R, Pira C, Rettaroli A, Ruoso G, Taffarello L and Tocci S 2020 Rev. Sci. Instrum. 91 094701
[18] CST Studio Suite 2021 December 2020 Dassault Systèmes Paris, France https://www.3ds.com/products/simulia/cst-studio-suite
[19] Youn S W 2017 2nd Workshop on Microwave Cavities and Detectors for Axion Research, January 10-13, 2017, California, USA |
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