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Origin of Elements & Cosmic Evolution 2025

9–14 Nov 2025
Peng Huanwu Collaborative Center for Research and Education, BUAA
Asia/Shanghai timezone

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Session

Talks

13 Nov 2025, 08:30
6th floor meeting room (Peng Huanwu Collaborative Center for Research and Education, BUAA)

6th floor meeting room

Peng Huanwu Collaborative Center for Research and Education, BUAA

Baiyan Bldg, North 4th Ring Road Middle, No. 238, Beijing, China

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  1. 17. Ejecta from nucleosynthesis events and their flows
    Roland Diehl
    13/11/2025, 08:30
  2. 34. The r-process elements enhanced stars with Galactic disk origins
    Hongliang Yan (National Astronomical Observatories, CAS)
    13/11/2025, 09:00
  3. 19. Imprints of Galactic Environments on Chemical Evolution
    Eda Gjergo (Nanjing University)
    13/11/2025, 09:30
  4. 46. Galactic chemical evolution in 3D
    Nicholas Storm (Max-Planck-Institute for Astronomy)
    13/11/2025, 09:50
  5. 20. Self-bound hybrid stars with strong phase transitions can relieve major compact star observation tensions
    Chen Zhang (Fudan University)
    13/11/2025, 10:50
  6. 21. Neutron stars as probes of dense QCD matter
    Sophia Han (T.D. Lee Institute / Shanghai Jiao Tong Univ)
    13/11/2025, 11:20
  7. 22. Symmetry energy effect on rotating neutron stars
    Xuhao Wu (Yanshan University)
    13/11/2025, 11:50
  8. 23. Nova brevis from magnetar giant flares: a new window on neutron star crusts
    Jiahang Zhong (Peking University)
    13/11/2025, 12:05
  9. 24. Neutrino Scattering in Nuclear Physics
    Myun-ki Cheoun (Soongsil University)
    13/11/2025, 14:00
  10. 25. On the Energetic Role of Forward Neutrino Scattering in CCSN Models
    Tatsushi Shima (Research Center for Nuclear Physics, Osaka University)
    13/11/2025, 14:30
  11. 26. Proton-rich production of lanthanides: the νi process
    Xilu Wang (Institute of High Energy Physics, Chinese Academy of Sciences)
    13/11/2025, 14:50
  12. 27. Contribution of Kilonovae to diffuse MeV Gamma-ray background
    PRANTIK SARMAH (Institute of High Energy Physics, Beijing)
    13/11/2025, 15:10
  13. 28. Nuclear de-excitation lines as a probe of low-energy cosmic rays
    Bing Liu (Purple Mountain Observatory, CAS)
    13/11/2025, 15:25
  14. 29. Lithium in the cosmos: old and rare and fragile
    Andreas Korn (Uppsala University)
    13/11/2025, 16:00
  15. 30. Stellar Atmospheric Parameters and Elemental Abundances from LAMOST Low-resolution Spectra with DD-PAYNE (Online)
    Meng Zhang (National Astronomical Observatories, CAS)
    13/11/2025, 16:30
  16. 31. One Element, Two Tracks: Age-Resolved Phosphorus Variation in the Young side of Milky Way (Online)
    Mingjie Jian (Stockholm University)
    13/11/2025, 16:50
  17. 32. Asetroseismology can give good ages for stars
    Tanda Li (Beijing Normal University)
    13/11/2025, 17:10
  18. 33. Chemo-chronology of the metal-poor Milky Way halo via asteroseismology
    Chenxi Wang (Nanjing University)
    13/11/2025, 17:30
  19. 18. Nucleosynthesis revealed from high-z galaxies and gas
    Siwei Zou (National Astronomical Observatories Of China (NAOC))
    14/11/2025, 08:30
  20. 35. Neutron-capture in the wild: Constraining r-process nucleosynthesis through metal-poor stars in the Milky Way (Online)
    Vinicius M Placco (NSF NOIRLab)
    14/11/2025, 08:50
  21. 36. Constraining r-process sites : [Th/Eu] in moderately metal-poor stars
    Kurumi Furutsuka (University of Hyogo)
    14/11/2025, 09:20
  22. 53. Meaurement of neutron capture cross section and its implication for astrophysics
    Suyalatu Zhang (Inner Mongolia Minzu University)
    14/11/2025, 09:35
  23. 38. Nuclear Structure and Dynamics from Stable Nuclei to Stellar Environments
    Nils Paar (University of Zagreb)
    14/11/2025, 10:15
  24. 48. Perspective on cosmos p-nuclei studies with the SLEGS gamma-ray source
    Prof. Jianjun HE (Fudan University)
    14/11/2025, 10:45
  25. 51. Toward astrophysics-driven nuclear-reaction experiments for Supernova nucleosynthesis
    Nobuya Nishimura (Kogakuin University)
    14/11/2025, 11:15
  26. 41. Clocked X-ray Bursters and New Aspects
    Akira Dohi (RIkagaku KENkyusho/Institute of Physical and Chemical Research)
    14/11/2025, 13:00
  27. 42. Indications of a Nuclear Urca Mechanism in the X-ray Superburster MAXI J1752−457
    Hao Huang (Institute of Modern Physics, CAS / Riken)
    14/11/2025, 13:30
  28. 43. Properties of Quark Star Merger Ejecta and the Observational Signature
    Zhiqiang Miao (TSUNG-DAO LEE Institute)
    14/11/2025, 13:45
  29. 39. Effects of beyond mean field approximation and tensor forces on Gamow-Teller and β decay of magic nuclei
    Hiroyuki Sagawa (University of Aizu)
    14/11/2025, 14:35
  30. 49. Supernova neutrino and JUNO
    Yufeng Li (Institute of High Energy Physics, CAS)
    14/11/2025, 15:05
  31. 50. Large neutron-to-proton conversion in light nuclear reactions at relativistic energies
    Baohua Sun (Beihang University)
    14/11/2025, 15:35
  32. 40. Nuclear weak rates for astrophysics based on the shell-model approach
    Toshio Suzuki (Nihon University)
    14/11/2025, 16:15
  33. 52. Nuclear reactions for nuclear astropysics and effective field theories
    Shung-Ichi Ando (Sunmoon University and Daegu University)
    14/11/2025, 16:45
  34. 37. Recent Studies on r-process Nuclear Cosmochronology
    Xinhui Wu (Fuzhou University)
    14/11/2025, 17:05
  35. 54. Charge-exchange reactions and the applications
    Bingshui Gao (Institute of Modern Physics)
    14/11/2025, 17:25
  36. 47. Modelling the Galactic Chemical Evolution of Dwarf Galaxies IC 10 and IC 1613: Unique r-Process Laboratories?
    GURUPRASAD YAGADEVAN (Wrocław University of Science and Technology,)
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