The opto-mechanics of the "Gravitational Reference System" for the LISA mission at PDR
Dr. Carlo Zanoni
INFN
Day
Tuesday · 2026-10-13
Time
3:20 PM - 4:20 PM
Track
General / Plenary
Session
Exhibition and Poster Session-2
Venue
ICSO 2026 Conference Venue
Track indicates the session hall. Refer to the on-site programme board for the exact room number and any last-minute room changes.
In 30 seconds
The Gravitational Reference System (GRS) acts as the heart of the LISA mission, using free-falling test masses to detect gravitational waves in the mHz frequency range. This design emphasizes the opto-mechanical integration of the test mass as an interferometer mirror, focusing on extreme stability and low acceleration noise. The work details the current engineering status, building on the flight heritage of the LISA Pathfinder mission.
Topics & Subtopics
Source traceability
ID: icso26_151
Schedule facts reproduced from the published ICSO 2026 programme. Enrichment metadata is a discovery aid, not a scientific classification.