3–7 Jun 2019
Europe/Berlin timezone

Superconducting YBCO microwave cavity in a high magnetic field for axion dark matter search

3 Jun 2019, 10:30
20m
Main Lecture Hall (Physics Department)

Main Lecture Hall

Physics Department

ALU Freiburg, Physikalisches Institut Hermann-Herder-Str. 3
Oral Morning 11

Speaker

Mr Danho Ahn (Institute for Basic Science, Center for Axion and Precision Physics Research, KAIST)

Description

Maintaining high Q-factor of the superconducting cavity in a strong magnetic field at gigahertz frequencies is a crucial component in a highly sensitive axion detection system and at the same time, a largely unexplored and challenging task. The natural choice of material for the superconducting cavity to be placed in a high magnetic field is a high-temperature superconductor (HTS) with a high critical field (>100 T) and a high depinning frequency (>10GHz). The deposition, however, of a high-quality, grain-aligned HTS film on a three-dimensional surface is technically difficult. IBS/CAPP has fabricated a polygon-shaped resonant cavity with commercial YBCO tapes covering the entire inner wall and measured the Q-factor at 4 K at 6.9 GHz as a function of an external DC magnetic field. We present the microwave measurement of the YBCO cavity (TM010 mode) which shows that the Q factor of the cavity do not degrade until 8 Tesla. This result indicates the possibility of realizing a high Q-factor superconducting cavity in a high magnetic field for axion search.

Primary author

Mr Danho Ahn (Institute for Basic Science, Center for Axion and Precision Physics Research, KAIST)

Co-authors

Prof. Dojun Youm (KAIST) Mr Doyu Lee (KAIST) Dr Jhinhwan Lee (IBS CALDES) Dr Ohjoon Kwon (Institute for basic science) SungWoo YOUN (CAPP/IBS) Dr Wonjun Jang (IBS/QNS) Dr Woohyun Chung (IBS/CAPP) Prof. Yannis Semertzidis (IBS/CAPP)

Presentation materials