Exploring the sensitivity of next generation gravitational wave detectors
The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe
|Collections||ANU Research Publications|
|Source:||Classical and Quantum Gravity|
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