Conveners
Session 4
- 雷 武
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Prof. 玉峰 李 (中国科学院高能物理研究所)18/10/2025, 16:10
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Prof. 永成 吴 (南京师范大学)18/10/2025, 16:30
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Prof. 成成 韩 (中山大学)18/10/2025, 16:50
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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...
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Prof. 万哲 冯 (天津大学)18/10/2025, 17:30
U(1) dark sectors accommodating viable dark matter candidate(s) will be discussed, including the evolution of dark particles, interplay between multiple hidden sectors, possible extended neutrino sectors, and gravitational wave generations. When the additional U(1) symmetry undergoes spontaneous breaking, the dark sector often exhibits a characteristic phase transition pattern capable of...
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