2025年紫金山暗物质研讨会

Name: 2025年紫金山暗物质研讨会
Start: 2025-10-17T09:00:00+08:00
End: 2025-10-21T17:00:00+08:00
Location: 烟台东山宾馆

17–21 Oct 2025

烟台东山宾馆

Asia/Shanghai timezone

Contribution List

22. Axion dark matter from topological defects

Prof. 立功边 (重庆大学)

Session 5

23. Axion Star Tidal Effects and Bosenova

Prof. 宇高 (高能所)

Session 1

21. Constraints on Strongly-Interacting Dark Matter from the James Webb Space Telescope

Prof. 佩之杜 (中国科学技术大学)

Session 1

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...

57. Dark matter searches with low-energy cosmic antinuclei

Prof. Mengjiao Xiao (上海交通大学)

GAPS实验组

6. Dark Photon Dark Matter Detection  with Radio Telescopes

Prof. 佳刘 (北京大学)

Session 1

24. Detection of ALPs with black hole superradiance

Prof. 宏张 (山东大学)

Session 1

44. Dilution Effect on Freeze-in Dark Matter from a Phase Transition

Prof. 阳张 (河南师范大学)

Session 1

41. Dynamical evolutions in globular clusters and dwarf galaxies

Prof. 益鸣钟 (香港城市大学)

Session 1

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...

4. First Direct Observation of Migdal Effect in Neutral Projectiles

Prof. 倩刘 (中国科学院大学)

Session 1

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...

25. Glueball Dark Matter

Prof. 志伟王 (电子科大)

Session 1

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...

11. Gravitational wave spectrums arising from dark matters

Prof. 伟晁 (北京师范大学)

Session 1

29. Heating effects of fuzzy dark matter in galaxies

Prof. Peng-Fei Yin (Institute of High Energy)

Session 1

33. Mapping Dark Matter in the Milky Way

Prof. 岚张 (国家天文台)

Session 1

12. Novel Light Dark Matter Detection with Quantum Parity Detector Using Qubit Arrays

Prof. Ningqiang Song (中科院理论物理所)

Session 1

45. PandaX实验进展

Prof. 月孟 (上海交通大学)

Session 1

PandaX实验

9. Probing Dark Matter with Gravitational-Wave Laser Interferometers in Space

Prof. 勇汤 (中国科学院大学)

Session 1

15. Probing nonthermal dark matter through large-scale structure observations

Prof. 成成韩 (中山大学)

Session 1

46. Recent status and prospects of CDEX @CJPL

Prof. Li-Tao Yang (清华大学)

Session 1

48. RECODE program for reactor neutrino CEvNS detection and Dark Matter

Prof. 永成吴 (南京师范大学)

Session 1

17. Searching for ALP DM in Alkali-Noble-Gas Haloscopes

Prof. 小平王 (北京航空航天大学)

Session 1

16. Searching for long-lived particles at Belle II

Prof. Zeren (泽人) Wang (王) (合肥工业大学)

Session 1

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...

13. Supernova Constraints on Lepton Flavor Violating Axions

Prof. 佐伟刘 (南京大学)

Session 1

5. talk title

Prof. 韶锋葛 (上海交通大学)

Session 1

10. talk title

Prof. 永超张 (东南大学)

Session 1

14. talk title

Prof. 玉峰李 (中国科学院高能物理研究所)

Session 1