First Scan Search for Dark Photon Dark Matter with a Tunable Superconducting Radio-Frequency Cavity

被引:1
|
作者
Tang, Zhenxing [1 ,2 ]
Wang, Bo [3 ]
Chen, Yifan [4 ]
Zeng, Yanjie [5 ,6 ]
Li, Chunlong [5 ]
Yang, Yuting [5 ,6 ]
Feng, Liwen [1 ,7 ]
Sha, Peng [8 ,9 ,10 ]
Mi, Zhenghui [8 ,9 ,10 ]
Pan, Weimin [8 ,9 ,10 ]
Zhang, Tianzong [1 ]
Jin, Yirong [11 ]
Hao, Jiankui [1 ,7 ]
Lin, Lin [1 ,7 ]
Wang, Fang [1 ,7 ]
Xie, Huamu [1 ,7 ]
Huang, Senlin [1 ,7 ]
Shu, Jing [1 ,2 ,12 ]
机构
[1] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
[2] Beijing Laser Accelerat Innovat Ctr, Huairou, Beijing 101400, Peoples R China
[3] Univ Chinese Acad Sci, Int Ctr Theoret Phys Asia Pacific, Beijing 100190, Peoples R China
[4] Niels Bohr Inst, Niels Bohr Int Acad, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[5] Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
[6] Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
[7] Peking Univ, Inst Heavy Ion Phys, Beijing 100871, Peoples R China
[8] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
[9] Chinese Acad Sci, Key Lab Particle Accelerat Phys & Technol, Beijing 100049, Peoples R China
[10] Chinese Acad Sci, Inst High Energy Phys, Ctr Superconducting RF & Cryogen, Beijing 100049, Peoples R China
[11] Beijing Acad Quantum Informat Sci, Beijing 100193, Peoples R China
[12] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
基金
中国国家自然科学基金;
关键词
Dark photons have emerged as promising candidates for dark matter; and their search is a top priority in particle physics; astrophysics; and cosmology. We report the first use of a tunable niobium superconducting radio-frequency cavity for a scan search of dark photon dark matter with innovative data analysis techniques. We mechanically adjusted the resonant frequency of a cavity submerged in liquid helium at a temperature of 2 K; and scanned the dark photon mass over a frequency range of 1.37 MHz centered at 1.3 GHz. Our study leveraged the superconducting radio-frequency cavity's remarkably high quality factors of approximately 1010; resulting in the most stringent constraints to date on a substantial portion of the exclusion parameter space on the kinetic mixing coefficient ϵ between dark photons and electromagnetic photons; yielding a value of ϵ © 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the https://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title; journal citation; and DOI. Funded by SCOAP3;
D O I
10.1103/PhysRevLett.133.021005
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Dark photons have emerged as promising candidates for dark matter, and their search is a top priority in particle physics, astrophysics, and cosmology. We report the first use of a tunable niobium superconducting radio-frequency cavity for a scan search of dark photon dark matter with innovative data analysis techniques. We mechanically adjusted the resonant frequency of a cavity submerged in liquid helium at a temperature of 2 K, and scanned the dark photon mass over a frequency range of 1.37 MHz centered at 1.3 GHz. Our study leveraged the superconducting radio-frequency cavity's remarkably high quality factors of approximately 10(10), resulting in the most stringent constraints to date on a substantial portion of the exclusion parameter space on the kinetic mixing coefficient & varepsilon; between dark photons and electromagnetic photons, yielding a value of & varepsilon; <2.2 x 10(-16).
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页数:7
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