2022
DOI: 10.1103/physrevapplied.17.l061005
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Biaxially Textured YBa2Cu3O7x Microwave Cavity in a High Magnetic Field for a Dark-Matter Axion Search

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Cited by 13 publications
(4 citation statements)
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“…Ahn et al observed similar field behaviors at small magnetic fields when characterizing their YBCO tape coated axion cavity. They attributed the magnetization to the Ni-9W metallic layer [22]. We have demonstrated that the peak at small magnetic fields is governed by the field response of the buffer layers [23], which after delamination remain in patches on the superconducting surface as can be seen in figure 7(a).…”
Section: Radio-frequency Measurementsmentioning
confidence: 99%
“…Ahn et al observed similar field behaviors at small magnetic fields when characterizing their YBCO tape coated axion cavity. They attributed the magnetization to the Ni-9W metallic layer [22]. We have demonstrated that the peak at small magnetic fields is governed by the field response of the buffer layers [23], which after delamination remain in patches on the superconducting surface as can be seen in figure 7(a).…”
Section: Radio-frequency Measurementsmentioning
confidence: 99%
“…In 2019, CAPP has solved the problem by attaching the well-grown 2-dimensional REBCO film directly to the inner wall of a 3-dimensional cavity. CAPP developed a prototype cavity in which the TM 010 mode resonated at 6.9 GHz using HTS tape and achieved a Q-factor six times higher than that of copper resonators at 4 K and 8 T magnetic field [283], as shown in Fig 22 . A second-generation cavity with a larger volume and a sapphire tuning system was then created to achieve a Q-factor of half a million and used in the physics run of axion search in 2021. Finally, CAPP's third-generation superconducting cavity development has achieved a Q-factor of order of 10 7 , which is 10 times the axion Q-factor, even in an 8 T magnetic field.…”
Section: Axion Searching Experiments At Ibs-cappmentioning
confidence: 99%
“…Figure 22: (a) Photo of CAPP's prototype superconducting cavity (b) Q-factor measurements of CAPP's 1st generation prototype superconducting cavity. These are imported from figure 1, 4 of[283] …”
mentioning
confidence: 99%
“…A frequency range of 30 GHz (corresponding to axion masses 330-460 µeV) could be covered with ∼ 3000 exposures. Assuming that a NEP of 3 × 10 −20 W/ √ Hz can be achieved with future technology and one could in principle gain an order of magnitude on the Q 0 using superconducting cavities [107], sensitivity down to g aγ ≈ 2 × 10 −13 GeV −1 can be achieved proofs JCAP_035P_0622 in a single exposure of ∼ 1 day. The mass range 330-460 µeV could therefore be probed on a total measuring time of ∼ 8 years (which can be split among several instruments with haloscopes build for different frequency ranges), shown by the region bounded by a thick black solid line in figure 12.…”
Section: Projected Axion Sensitivitymentioning
confidence: 99%