期刊
CLASSICAL AND QUANTUM GRAVITY
卷 34, 期 4, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/1361-6382/aa51f4
关键词
gravitational waves; cosmic explorer; LIGO
类别
资金
- National Science Foundation [PHY-0757058]
- [PHY-0823459]
- STFC [ST/I001026/1, ST/N000080/1, ST/J000302/1, ST/I006242/1, ST/L000954/1, ST/J000019/1, ST/J000345/1, ST/N005716/1, ST/N000072/1, ST/N000064/1, ST/L003465/1, PP/C505791/1, Gravitational Waves, PPA/G/S/2002/00652, ST/N00003X/1, PP/F00110X/1, ST/M005844/1, ST/N005481/1, ST/L000962/1, ST/L000911/1, ST/L000946/1, ST/L000326/1, ST/N005406/1, ST/I006285/1, ST/N000633/1, ST/I000887/1, 1653089, ST/J000361/1, ST/N005430/1, ST/K000845/1, ST/N005422/1, ST/I006269/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/N00003X/1, ST/L000911/1 Gravitational Waves, ST/I006269/1, ST/I001026/1, ST/L000954/1, ST/P000258/1, Gravitational Waves, ST/L000326/1, PPA/G/S/2002/00652, ST/L000911/1, ST/L000946/1, ST/N005481/1, ST/J000361/1, ST/N005422/1, ST/L003465/1, ST/N000633/1, ST/M005844/1, PP/F00110X/1, ST/I006269/1 Gravitational Waves, ST/J000302/1, ST/J000019/1, ST/J000302/1 Gravitational Waves, ST/N005716/1, ST/N000080/1, ST/N005406/1, ST/K000845/1, ST/I006242/1, ST/N000072/1, ST/I001026/1 Gravitational Waves] Funding Source: researchfish
- Direct For Education and Human Resources
- Division Of Human Resource Development [1242090] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [1506497, 1607709, 1505779, 1308527, 1404139, 1506360, 1505629] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [1205882, 1505308, 1607585, 1505373] Funding Source: National Science Foundation
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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