13–16 Oct 2025
Asia/Shanghai timezone

Contribution List

30 out of 30 displayed
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  1. Alessandro Vicini (University of Milan)
    13/10/2025, 08:30
  2. Alessandro Vicini (University of Milan)
    13/10/2025, 09:30
  3. Alessandro Vicini (University of Milan)
    13/10/2025, 11:00
  4. Sven Heinemeyer (IFT/IFCA (CSIC))
    13/10/2025, 13:30
  5. Maria Martinez (CAPA/Zaragoza University)
    13/10/2025, 15:30
  6. Alessandro Vicini (University of Milan)
    14/10/2025, 08:30
  7. Alessandro Vicini (University of Milan)
    14/10/2025, 09:30
  8. Alessandro Vicini (University of Milan)
    14/10/2025, 11:00
  9. Sven Heinemeyer (IFT/IFCA (CSIC))
    14/10/2025, 13:30
  10. Huilin Qu (CERN)
    14/10/2025, 15:30
  11. Maria Martinez (CAPA/Zaragoza University)
    14/10/2025, 18:30
  12. Alessandro Vicini (University of Milan)
    15/10/2025, 08:30
  13. Alessandro Vicini (University of Milan)
    15/10/2025, 09:30
  14. Sven Heinemeyer (IFT/IFCA (CSIC))
    15/10/2025, 11:00
  15. Alessandro Vicini (University of Milan)
    15/10/2025, 13:30
  16. Yue Meng (Shanghai Jiao Tong University)
    15/10/2025, 15:30
  17. Alessandro Vicini (University of Milan)
    16/10/2025, 08:30
  18. Huilin Qu (CERN)
    16/10/2025, 09:30
  19. Alessandro Vicini (University of Milan)
    16/10/2025, 11:00
  20. Ning Zhou (Shanghai Jiao Tong University)
    16/10/2025, 13:30
  21. Huilin Qu (CERN)
    16/10/2025, 15:30
  22. Alessandro Vicini (University of Milano)
  23. Alessandro Vicini (University of Milano)
  24. Alessandro Vicini (University of Milano)
  25. Alessandro Vicini (University of Milano)
  26. Alessandro Vicini (University of Milano)
  27. Prof. Shao-Feng Ge (TDLI-SJTU)

    We propose practical ways of differentiating the various (Breit-Wigner, theoretical, and energy-dependent) resonance schemes of unstable particles at lepton colliders. First, the energy-dependent scheme can be distinguished from the other two by fitting the $Z$ lineshape scan and forward-backward asymmetries at LEP and future lepton colliders with the $Z$ mass $m_Z$, decay width $\Gamma_Z$,...

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