High-Q Microwave Dielectric Resonator for Axion Dark-Matter Haloscopes

被引：11

作者：

Di Vora, R. ^{[1
,2
]}

Alesini, D. ^{[3
]}

Braggio, C. ^{[1
,4
,5
]}

Carugno, G. ^{[1
]}

Crescini, N. ^{[6
]}

D'Agostino, D. ^{[7
]}

Di Gioacchino, D. ^{[3
]}

Falferi, P. ^{[8
,9
]}

Gambardella, U. ^{[7
]}

Gatti, C. ^{[3
]}

Iannone, G. ^{[7
,10
]}

Ligi, C. ^{[3
]}

Lombardi, A. ^{[6
]}

Maccarrone, G. ^{[3
]}

Ortolan, A. ^{[6
]}

Pengo, R. ^{[6
]}

Rettaroli, A. ^{[3
,11
]}

Ruoso, G. ^{[6
]}

Taffarello, L. ^{[1
]}

Tocci, S. ^{[3
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Padova, Via Francesco Marzolo 8, I-35131 Padua, Italy

[2] Univ Siena, Dipartimento Sci Fis Terra & Ambiente, Via Roma 56, I-53100 Siena, Italy

[3] Ist Nazl Fis Nucl, Lab Nazl Frascati, Rome, Italy

[4] Univ Padua, Dipartimento Fis & Astron G Galilei, Padua, Italy

[5] Fermilab Natl Accelerator Lab, Superconducting Quantum Mat & Syst Ctr SQMS, Batavia, IL 60510 USA

[6] Ist Nazl Fis Nucl, Lab Nazl Legnaro, Padua, Italy

[7] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy

[8] CNR Fdn Bruno Kessler, Ist Foton & Nanotecnol, I-38123 Trento, Italy

[9] Ist Nazl Fis Nucl, TIFPA, Trento, Italy

[10] Univ Salerno, Dipartimento Fis ER Caianiello, Via Giovanni Paolo II 132, I-82084 Salerno, Italy

[11] Univ Roma Tre, Dipartimento Matemat & Fis, I-00100 Rome, Italy

来源：

PHYSICAL REVIEW APPLIED | 2022年 / 17卷 / 05期

关键词：

CP CONSERVATION;

D O I：

10.1103/PhysRevApplied.17.054013

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

The frequency band 1???15 GHz provides exciting prospects for resonant axion haloscopes as indicated by cosmological and astrophysical arguments. Among the challenges currently addressed to reach the required sensitivity, the development of high-quality factor cavities that tolerate multitesla fields plays a central role. We report a three-dimensional resonator based on a right-circular copper cavity with hollow cylinders that confine higher-order modes around the cylinder axis. Its effective volume at 10.3 GHz is 3.4 ?? 10???2 l, and under an 8-T field we measure an internal quality factor of more than nine million. A fine-tuning system limited to approximately 1-MHz range is tested, useful for understanding the conditions required to run a haloscope with a cavity exceeding the axion quality factor. The cavity parameters we report demonstrate the potential of this unique resonator to probe galactic dark-matter axion at scan rates exceeding 2 MHz/day when the cavity is readout by a quantum-limited receiver.

引用

页数：10

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