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BEGIN:VEVENT
DTSTAMP:20260523T194053Z
UID:https://www.cpfs.mpg.de/events/44898/2615573
DTSTART:20260305T140000Z
DTEND:20260305T160000Z
CLASS:PUBLIC
CREATED:20260224T113913Z
DESCRIPTION: Gravitational-wave detectors (GWDs) require extremely sensitiv
 e and compact sensors to detect and correct for seismic vibration. For fut
 ure detectors and upgrades of current ones\, even the best commercial sens
 ors do not meet the sensitivity requirements. This is because commercial s
 eismometers are designed to characterize the quietest places on Earth. How
 ever\, with the seismic attenuation systems used in GWDs\, we create envir
 onments that move much less than the Earth at the frequencies where we aim
  to detect a black hole or neutron star merger.\nVortragende(r): Joris van
  Heijningen
LAST-MODIFIED:20260507T080229Z
LOCATION:MPI CPfS\, Raum: Seminarraum 1 + 2
ORGANIZER;CN=Dr. Uri Vool:mailto:
SUMMARY:CPfS Seminar:  (Sub-)proton-scale vibration measurements for future
  terrestrial and lunar gravitational-wave detectors 
URL;VALUE=URI:https://www.cpfs.mpg.de/events/44898/2615573
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