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)
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15/06/2026, 13:00
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Angélique Lartaux (IJCLab)15/06/2026, 13:05
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Patrice Verdier (IP2I Lyon - IN2P3)15/06/2026, 13:25
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Michele Maggiore (University of Geneva, Switzerland)15/06/2026, 13:45
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Niels Warburton15/06/2026, 14:05
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Viola Sordini (CNRS France)15/06/2026, 14:25
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15/06/2026, 14:45
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15/06/2026, 15:30
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Michael Landry15/06/2026, 15:45
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Harsh Narola15/06/2026, 16:05
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15/06/2026, 16:25
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15/06/2026, 16:45
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15/06/2026, 17:10
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Shinji MIYOKI (Institute for Cosmic Ray Research, The University of Tokyo)18/06/2026, 10:00
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Gabriele Capoccia (INFN-PG)18/06/2026, 10:20Plenarytalk
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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Marco Vardaro18/06/2026, 10:40Plenarytalk
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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Stefan Hild18/06/2026, 10:55
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Jan Harms, Stefan Hild18/06/2026, 11:05
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Angélique Lartaux (IJCLab)18/06/2026, 11:25
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Dr Francesco Iacovelli (Johns Hopkins University), Mikhail Korobko, Ulyana Dupletsa (MBI), valeria sequino18/06/2026, 11:35
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18/06/2026, 11:55
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François Gautier (Laboratoire d'Acoustique de l'Université du Mans, UMR CNRS 6613)18/06/2026, 13:30Plenarytalk
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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Tomislav Andric18/06/2026, 13:45
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18/06/2026, 14:00
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Paul Laycock18/06/2026, 16:00
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Archisman Ghosh (Universiteit Gent), Marica Branchesi, Michela Mapelli, Paolo Pani18/06/2026, 16:20
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Andreas Rietbrock, Domenico D'Urso, Dr Wim Walk (Nikhef)18/06/2026, 16:40
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18/06/2026, 17:00
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18/06/2026, 17:20
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18/06/2026, 17:40
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Anna Green (Nikhef)19/06/2026, 10:00
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Luca Naticchioni19/06/2026, 10:10
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Jessica Steinlechner, alex amato (Maastricht University - Nikhef)19/06/2026, 10:20
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Disha Subhash Sawant19/06/2026, 10:30
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Yuliya Hoika (University of Warsaw)19/06/2026, 10:45
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Dorota Rosinska (University of Warsaw)19/06/2026, 11:05
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Lorenzo Aiello19/06/2026, 11:20Plenarytalk
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.
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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... -
19/06/2026, 11:40
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Michael Prouza, Michele Maggiore (University of Geneva, Switzerland)19/06/2026, 11:50