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Pushing the low and high-frequency detector sensitivity (below 10 and above 1kHz)

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If you have a question about this talk, please contact Nathan Steinle.

Gravitational-wave observations across multiple frequency bands will be the future of gravitational-wave astronomy, similar to the development of electromagnetic observations. In this talk, I will focus on ground-based detectors, and talk about the efforts in improving the detector sensitivity both at the low and high-frequency end of the spectrum. I will highlight two technologies: the 6D seismometer and the quantum filter. Apart from the application to gravitational-wave detections, these two also allow us to explore quantum behaviours of macroscopic objects and new principles of high-precision measurements.

This talk is part of the Astrophysics Talks Series series.

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