Abstract
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.
Original language | English (US) |
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Article number | 044001 |
Journal | Classical and Quantum Gravity |
Volume | 34 |
Issue number | 4 |
DOIs | |
State | Published - Jan 24 2017 |
Bibliographical note
Publisher Copyright:© 2017 IOP Publishing Ltd.
Keywords
- LIGO
- cosmic explorer
- gravitational waves