Document Type
Article
Department/Program
Physics
Journal Title
CLASSICAL AND QUANTUM GRAVITY
Pub Date
2-23-2018
Volume
34
Issue
4
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.
Recommended Citation
Abbott, B. P.; Abbott, R.; Abbott, T. D.; Abernathy, M. R.; Ackley, K.; Adams, C.; Addesso, P.; Adhikari, R. X.; Adya, V. B.; Affeldt, C.; Aggarwal, N.; Aguiar, O. D.; Ain, A.; Ajith, P.; Allen, B.; Altin, P. A.; Anderson, S. B.; Anderson, W. G.; Arai, K.; Araya, M. C.; Arceneaux, C. C.; Mikhailov, Eugeniy E.; Rew, H.; Romanov, G.; and Zhang, M., Exploring the sensitivity of next generation gravitational wave detectors (2018). CLASSICAL AND QUANTUM GRAVITY, 34(4).
10.1088/1361-6382/aa51f4
DOI
10.1088/1361-6382/aa51f4
