Conveners
Session 4
- 雷 武
Prof.
玉峰 李
(中国科学院高能物理研究所)
18/10/2025, 16:10
Prof.
永成 吴
(南京师范大学)
18/10/2025, 16:30
Prof.
成成 韩
(中山大学)
18/10/2025, 16:50
Prof.
Christina Gao
(南方科技大学)
18/10/2025, 17:10
Axion dark matter may couple to fermion spins through an effective oscillating magnetic field, the ``axion wind". Existing approaches for detecting axion wind via axion-electron coupling face sensitivity limitations due to the extremely weak pseudomagnetic field generated, typically a few times $10^{-18}$ tesla for $g_{ae} \sim 10^{-10}$. We propose to use ferrimagnetic flux concentrators to...
