15–19 Jun 2026
Europe/Rome timezone

Session

Plenary Session

15 Jun 2026, 13:00

Conveners

Plenary Session: Plenary Session

  • Angélique Lartaux (IJCLab)
  • Michele Maggiore (University of Geneva, Switzerland)

Plenary Session

  • Angélique Lartaux (IJCLab)
  • Michele Maggiore (University of Geneva, Switzerland)

Plenary Session

  • Michele Maggiore (University of Geneva, Switzerland)
  • Angélique Lartaux (IJCLab)

Plenary Session

  • Michele Maggiore (University of Geneva, Switzerland)
  • Angélique Lartaux (IJCLab)

Plenary Session

  • Angélique Lartaux (IJCLab)
  • Michele Maggiore (University of Geneva, Switzerland)

Plenary Session

  • Michele Maggiore (University of Geneva, Switzerland)
  • Angélique Lartaux (IJCLab)

Presentation materials

There are no materials yet.

  1. 15/06/2026, 13:00
  2. Angélique Lartaux (IJCLab)
    15/06/2026, 13:05
  3. Patrice Verdier (IP2I Lyon - IN2P3)
    15/06/2026, 13:25
  4. Michele Maggiore (University of Geneva, Switzerland)
    15/06/2026, 13:45
  5. Niels Warburton
    15/06/2026, 14:05
  6. Viola Sordini (CNRS France)
    15/06/2026, 14:25
  7. 15/06/2026, 14:45
  8. 15/06/2026, 15:30
  9. Michael Landry
    15/06/2026, 15:45
  10. Harsh Narola
    15/06/2026, 16:05
  11. 15/06/2026, 16:25
  12. 15/06/2026, 16:45
  13. 15/06/2026, 17:10
  14. Shinji MIYOKI (Institute for Cosmic Ray Research, The University of Tokyo)
    18/06/2026, 10:00
  15. Gabriele Capoccia (INFN-PG)
    18/06/2026, 10:20
    Plenary
    talk

    The CAOS international laboratory (Center for Gravitational Wave and Seismology Applications) of the University of Perugia, in collaboration with INFN and EGO and primarily funded by the ETIC (Einstein Telescope Infrastructure Consortium) project, is mainly designed to develop and test new technologies for the Einstein Telescope. The facility will focus on the development and fine-tuning of...

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  16. Marco Vardaro
    18/06/2026, 10:40
    Plenary
    talk

    The European third generation gravitational-wave detector Einstein Telescope will rely on cryogenics and silicon as mirror and suspension material to achieve unprecedented low-frequency sensitivity. Prototyping and characterisation of these new technologies on a system-level is needed to inform the design and future upgrades of the large-scale observatory. This is one of the mission of...

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  17. Stefan Hild
    18/06/2026, 10:55
  18. Jan Harms, Stefan Hild
    18/06/2026, 11:05
  19. Angélique Lartaux (IJCLab)
    18/06/2026, 11:25
  20. Dr Francesco Iacovelli (Johns Hopkins University), Mikhail Korobko, Ulyana Dupletsa (MBI), valeria sequino
    18/06/2026, 11:35
  21. 18/06/2026, 11:55
  22. François Gautier (Laboratoire d'Acoustique de l'Université du Mans, UMR CNRS 6613)
    18/06/2026, 13:30
    Plenary
    talk

    Among the noise sources affecting GW detectors, Newtonian noise of seismic, acoustic, or atmospheric origin could limit sensitivity at low frequencies, below a few tens of Hz. This presentation focuses on modeling acoustic Newtonian noise resulting from technical noise in caverns and experimental chambers. A significant contribution to these technical noises is specifically linked to the...

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  23. Tomislav Andric
    18/06/2026, 13:45
  24. 18/06/2026, 14:00
  25. Paul Laycock
    18/06/2026, 16:00
  26. Archisman Ghosh (Universiteit Gent), Marica Branchesi, Michela Mapelli, Paolo Pani
    18/06/2026, 16:20
  27. Andreas Rietbrock, Domenico D'Urso, Dr Wim Walk (Nikhef)
    18/06/2026, 16:40
  28. 18/06/2026, 17:00
  29. 18/06/2026, 17:20
  30. 18/06/2026, 17:40
  31. Anna Green (Nikhef)
    19/06/2026, 10:00
  32. Luca Naticchioni
    19/06/2026, 10:10
  33. Jessica Steinlechner, alex amato (Maastricht University - Nikhef)
    19/06/2026, 10:20
  34. Disha Subhash Sawant
    19/06/2026, 10:30
  35. Yuliya Hoika (University of Warsaw)
    19/06/2026, 10:45
  36. Dorota Rosinska (University of Warsaw)
    19/06/2026, 11:05
  37. Lorenzo Aiello
    19/06/2026, 11:20
    Plenary
    talk

    Optical aberrations represent a major sensitivity bottleneck for current and future gravitational wave interferometers, as they limit stable operation at the high optical powers required to reduce quantum noise.
    The non axisymmetric component of these aberrations is not currently corrected in Advanced GW detectors, since its impact remains negligible at present power levels. However, with...

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  38. 19/06/2026, 11:40
  39. Michael Prouza, Michele Maggiore (University of Geneva, Switzerland)
    19/06/2026, 11:50
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