Exploring the sensitivity of next generation gravitational wavedetectors
California Institute of Technology · Louisiana State University · +94 more institutions
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Abstract
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.
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722Topics & keywords
Topics
Keywords
- Physics
- Gravitational wave
- Detector
- Sensitivity (control systems)
- Gravitational-wave observatory
- Einstein Telescope
- Universe
- Gravitational-wave astronomy
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Funding
- NSNational Science FoundationAwards: 0757058, 0823459, PHY-0757058, PHY-0823459
- MIMassachusetts Institute of TechnologyAward: PHY-0757058
- CICalifornia Institute of Technology
- SAScience and Technology Facilities CouncilAwards: ST/I006242/1, ST/N000064/1, ST/P000258/1, ST/L000946/1, PP/F00110X/1, ST/I006269/1, ST/I000887/1, ST/N005406/1, ST/L003465/1, Gravitational Waves, ST/J000345/1, ST/I006285/1, ST/I001026/1, ST/N000633/1, ST/N00003X/1, ST/L000911/1, ST/L000954/1, ST/L000326/1, ST/M005844/1, 1653089, ST/L000962/1, ST/K000845/1, ST/N005716/1, ST/N005422/1, ST/J000019/1, ST/N005481/1, ST/N000072/1, ST/J000361/1, ST/N000080/1, ST/N005430/1