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2023 弥散伽马射线与宇宙线研讨会暨 “宇宙线起源”青年团队年度总结会议

21–24 Oct 2023
合肥融创美居酒店
Asia/Shanghai timezone

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Contribution List

28 out of 28 displayed
  1. 4. Opening/Welcome
    22/10/2023, 09:00
  2. 48. 青年团队项目总体进展汇报
    Qiang Yuan (PMO)
    22/10/2023, 09:10
  3. 50. DAMPE实验进展
    Chuan Yue
    22/10/2023, 09:50
  4. 51. LHAASO KM2A diffuse
    Rui Zhang
    22/10/2023, 10:10
  5. 21. LHAASO gamma-ray overview
    Cong Li
    22/10/2023, 14:00
  6. 27. LHAASO WCDA diffuse
    Peipei Zhang
    22/10/2023, 14:25
  7. 47. Search for VHE Gamma-Rays from the Northern Fermi Bubble with LHAASO
    思达 李 (中国科学院上海天文台)
    22/10/2023, 14:50

    The Fermi Bubbles are a pair of bubble-like structures symmetric to the galactic center, which are assumed to be morphologically formed by strong energy releasing events happened million years ago. Regarding the emitted Gamma-Rays, high energy radiation processes like hadronic or leptonic emissions accompanying the outflows are responsible for the origin of the emission. As predicted by...

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  8. 30. DAMPE gamma-ray overview
    Zhaoqiang Shen (PMO)
    22/10/2023, 15:15
  9. 55. A study of Forbush Decreases effects with DAMPE experiment
    文昊 李 (中国科学院紫金山天文台)
    22/10/2023, 15:40

    Forbush Decreases (FDs) refer to the rapid decrease and slow recovery in the observed intensity of galactic cosmic rays (GCRs). They are primarily caused by active solar events that sweep low-energy galactic cosmic rays away from Earth. Different characteristics of FDs have been observed through various experiments. The observations are collected mostly from worldwide ground-based Neutron...

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  10. 32. Investigating the distribution of cosmic rays using diffuse gamma-rays
    Ruizhi Yang
    22/10/2023, 16:30
  11. 33. On the Origin of Galactic Diffuse TeV-PeY Emission: Insight from LHAASO and IceCube
    Kai Yan
    22/10/2023, 16:55
  12. 26. Multi-messenger Study of Galactic Diffuse Emission with LHAASO and IceCube Observations
    苏杰 林 (Sun Yat-Sen University)
    22/10/2023, 17:20

    With the breakthrough in PeV gamma-ray astronomy brought by the LHAASO experiment, the high-energy sky is getting richer than before. Lately, LHAASO Collaboration reported the observation of a gamma-ray diffuse emission with energy up to the PeV level from both the inner and outer Galactic plane. In these spectra, there is one bump that is hard to explain by the conventional cosmic-ray...

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  13. 35. 宇宙线传播研究进展
    Xiaojun Bi
    22/10/2023, 17:45
  14. 36. DAMPE p, He 观测
    Chuan Yue
    23/10/2023, 09:00
  15. 37. Measurements of the carbon and oxygen fluxes in cosmic rays with the DAMPE experiment
    Dr Yifeng Wei (University of Science and Technology of China)
    23/10/2023, 09:25
  16. 38. DAMPE 次级粒子观测
    Zhanfang Chen
    23/10/2023, 09:50
  17. 39. The measurements of all-particle energy spectrum and mean logarithmic mass of cosmic rays from 0.3 to 30 PeV with LHAASO-KM2A
    恒英 张 (中国科学院高能物理研究所)
    23/10/2023, 10:45
  18. 40. LHAASO 宇宙线能谱和组分
    Shoushan Zhang
    23/10/2023, 11:10
  19. 41. LHAASO WCDA各向异性
    Dongxu Sun
    23/10/2023, 11:35
  20. 42. LHAASO KM2A各向异性
    Jiayin He
    23/10/2023, 12:00
  21. 43. Cosmic Ray Acceleration and Feedback at the Galactic Center
    Fulai Guo (Shanghai Astronomical Observatory, Chinese Academy of Sciences)
    23/10/2023, 14:00
  22. 44. 基于宇宙线多信使反常观测研究其共同起源问题
    Yiqing Guo
    23/10/2023, 14:25
  23. 52. 宇宙线大尺度各向异性起源
    Wei Liu
    23/10/2023, 14:50
  24. 54. Study of propagation origin of the knee structure in cosmic ray energy spectrum using large-scale anisotropy
    Hua Yue (Institute of High Energy Physics, CAS)
    23/10/2023, 15:15

    The origin of the knee structure in cosmic ray (CR) energy spectrum remains unresolved. Various types of models have been proposed to explain it, which can be distinguished as acceleration origin (due to the limitation of the maximum possible CR energy by Galactic sources), propagation origin (because of the transition from slow to fast diffusion of Galactic CRs), interaction origin and local...

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  25. 25. Searching for Magnetic Selected UHECR Structures
    Haoning He (PMO)
    23/10/2023, 15:40

    The Pierre Auger Observatory (PAO) collaboration has reported more than 2600 ultrahigh-energy cosmic rays (UHECRs) lately. Adopting a universal model with one source and energy-dependent magnetic deflections, we found the magnetic selected UHECR structure from the PAO public data around the direction of Centaurus A.

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  26. 53. Study of Galactic diffusion coefficient with the spectrum features of UHECR
    Dan li (IHEP)
    23/10/2023, 16:05

    The Auger Collaboration has recently published the energy spectrum of cosmic rays above 1 EeV, which exhibits interesting features. These spectrum features provide an opportunity to investigate the propagation of ultra-high-energy cosmic rays (UHECRs). In this study, we have developed a model that incorporates the dip model for UHECRs in the extragalactic propagation, while accounting for the...

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  27. 3. DAMPE 项目总体进展报告
  28. 28. HAWC diffuse
    Hao Zhou