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Title: The Lunar Gravitational-wave Antenna Abstract: Gravitational-wave (GW) observations with the Virgo and LIGO detectors have revolutionized astronomy and physics. With more than 300 detections today, we can start to study in greater detail the properties of black holes and their distribution in our Universe. The observation of the merger of two neutron stars in 2017 has led to the greatest astronomical campaign in human history with numerous publications dedicated to its study. Despite these outstanding achievements, the field is only in its infancy, and new revolutionary instruments are underway like the space-based LISA mission or the proposed Einstein Telescope. Even then, GW detectors will only observe a small portion of all possibly detectable GW sources in our Universe, and researchers have started to develop new detector concepts to further extend the scientific reach of GW detectors. Among these concepts is the Lunar Gravitational-wave Antenna (LGWA). The Moon itself acts like an antenna to GWs by starting to ring like a bell when a GW passes. A transducer needs to be built to read out the vibrations of the Moon. The Moon provides close to ideal conditions for LGWA, and it might well be the only place in our solar system where a detector like LGWA can ever be realized. Speaker: Jan Harms - Gran Sasso Science Institute, Italy Date and Time: December 10th, 2025 - 12pm GMT