17–21 Oct 2025
烟台东山宾馆 6 号楼
Asia/Shanghai timezone

Contribution List

53 out of 53 displayed
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  1. Prof. 丽桃 杨 (清华大学)
    18/10/2025, 09:00
  2. Prof. 月 孟 (上海交通大学)
    18/10/2025, 09:20
  3. Prof. 飞 高 (清华大学)
    18/10/2025, 09:40
  4. Prof. 倩 刘 (中国科学院大学)
    18/10/2025, 10:00

    The Migdal effect, a phenomenon in which a nucleus emits an electron following a perturbation, is considered one of the most sensitive methods for detecting sub-GeV dark matter to date. However, for over 80 years, direct observational evidence has been lacking. This presentation will showcase the gas pixel detector we designed for the direct observation of the Migdal effect, along with the...

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  5. Xiang LI (PMO)
    18/10/2025, 10:50

    DAMPE and VLAST实验组

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  6. Prof. 庆宏 曹 (北京大学)
    18/10/2025, 11:10
  7. Prof. 韶锋 葛 (上海交通大学)
    18/10/2025, 11:30
  8. Prof. 江浩 于 (中科院理论物理研究所)
    18/10/2025, 13:40
  9. Prof. 佳 刘 (北京大学)
    18/10/2025, 14:00
  10. Prof. 勇 汤 (中国科学院大学)
    18/10/2025, 14:20
  11. Prof. 雯宇 王 (北京工业大学)
    18/10/2025, 14:40
  12. Prof. 立功 边 (重庆大学)
    18/10/2025, 15:00
  13. Prof. 致廷 卢 (南京师范大学)
    18/10/2025, 15:20
  14. Prof. 玉峰 李 (中国科学院高能物理研究所)
    18/10/2025, 16:10
  15. Prof. 永成 吴 (南京师范大学)
    18/10/2025, 16:30
  16. Prof. 成成 韩 (中山大学)
    18/10/2025, 16:50
  17. 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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  18. 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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  19. Prof. 家信 韩
    19/10/2025, 08:30

    Many universal yet simple laws have been discovered describing the distributions of subhalos, including their initial and final mass functions and spatial distributions. Validating the fidelity of these laws against numerical effects and extending them to different cosmologies require physical understanding of their origins. In this talk, I will introduce an extremely simple idea to unify the...

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  20. Prof. 慧元 王 (中国科技大学)
    19/10/2025, 08:50
  21. Prof. 益鸣 钟 (香港城市大学)
    19/10/2025, 09:10

    We present a new two-fluid conduction scheme to simulate the evolution of an isolated, self-gravitating, equilibrium cluster of stars and collisionless dark matter on secular (gravothermal) timescales. We integrate the equations in Lagrangian coordinates via a second-order, semi-implicit algorithm, which is unconditionally stable when the mass of the lighter species is much less than that of...

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  22. Prof. 方周 姜 (北京大学)
    19/10/2025, 09:30
  23. Prof. 岚 张 (国家天文台)
    19/10/2025, 09:50
  24. Juntai Shen (上海交通大学)
    19/10/2025, 10:40

    前人的工作大多默认太阳邻域暗物质的速度服从麦克斯韦-玻尔兹曼分布,而近些年来对银河系早期主并合事件的研究表明,真实的速度分布会一定程度偏离标准暗晕模型,这对暗物质直接探测实验中的年度调制效应和排除曲线有一定的影响,从而影响对实验结果的解读。

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  25. Prof. 世鸿 廖 (国家天文台)
    19/10/2025, 11:00
  26. Prof. Peng-Fei Yin (Institute of High Energy)
    19/10/2025, 11:20
  27. Prof. 宏 张 (山东大学)
    19/10/2025, 11:40
  28. Prof. 佐伟 刘 (南京大学)
    19/10/2025, 13:40
  29. Prof. Ningqiang Song (中科院理论物理所)
    19/10/2025, 14:00
  30. Prof. 小平 王 (北京航空航天大学)
    19/10/2025, 14:20
  31. Prof. 宇 高 (高能所)
    19/10/2025, 14:40
  32. Prof. 永超 张 (东南大学)
    19/10/2025, 15:00
  33. Prof. 佩之 杜 (中国科学技术大学)
    19/10/2025, 15:20

    Direct detection searches for dark matter are insensitive to dark matter particles that have large interactions with ordinary matter, which are stopped in the atmosphere or the Earth’s crust before reaching terrestrial detectors. We use “dark” calibration images from the James Webb Space Telescope to derive novel constraints on sub-GeV dark matter candidates that scatter off electrons. In this...

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  34. Prof. 伟 晁 (北京师范大学)
    19/10/2025, 16:10
  35. Prof. 发朋 黄 (中山大学)
    19/10/2025, 16:30
  36. Prof. 志伟 王 (电子科大)
    19/10/2025, 16:50

    We explore a generic class of composite dark matter candidates arising from confining dark sectors, where phase transitions—especially deconfinement-confinement and chiral symmetry breaking—can generate stochastic gravitational waves. Using a combination of lattice results and effective field theory approaches such as the Polyakov Loop and PNJL models, we analyze the dynamics of these phase...

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  37. Prof. Zeren Simon (泽人) Wang (王) (合肥工业大学)
    19/10/2025, 17:10

    Searching for long-lived particles (LLPs) has emerged as an important research direction in the quest for physics beyond the Standard Model. Such searches can be performed at various terrestrial facilities including colliders, beam-dump experiments, and neutrino experiments. In this talk, I will focus on the ongoing Belle II experiment at the SuperKEKB collider in Tsukuba, Japan. I will...

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  38. Prof. 阳 张 (河南师范大学)
    19/10/2025, 17:30
  39. 宇根 林
    20/10/2025, 08:30
  40. 迈 乔
    20/10/2025, 08:50
  41. 春龙 李
    20/10/2025, 09:10
  42. 亮 谭
    20/10/2025, 09:30
  43. 朋龙 张
    20/10/2025, 09:50
  44. 瑞珈 张
    20/10/2025, 10:40
  45. 宏昕 王
    20/10/2025, 11:00
  46. 玉明 杨
    20/10/2025, 11:20
  47. 骁 王
    20/10/2025, 11:40
  48. 拿云 贾
    20/10/2025, 14:00
  49. 思媛 侯
    20/10/2025, 14:20
  50. Lily Zhang
    20/10/2025, 14:40
  51. 垠 吴
    20/10/2025, 15:00
  52. 子煊 刘
    20/10/2025, 15:20
  53. Prof. 木拉提 阿不都艾尼 (新疆大学)
    20/10/2025, 15:40