Exploring the sensitivity of next generation gravitational wave detectors
Author(s)
Aggarwal, Nancy; Barsotti, Lisa; Biscans, Sebastien; Buikema, Aaron; Donovan, Frederick J; Essick, Reed Clasey; Evans, M.; Fritschel, Peter K.; Gras, Slawomir; Isogai, Tomoki; Katsavounidis, Erotokritos; Kontos, Antonios; Libson, Adam A.; Lynch, Ryan Christopher; MacInnis, Myron E; Martynov, Denis; Mason, Kenneth R; Matichard, Fabrice; Mavalvala, Nergis; Miller, John; Mittleman, Richard K; Mohapatra, S. R. P.; Oelker, Eric Glenn; Shoemaker, David H; Tse, Maggie; Vaulin, Ruslan; Vitale, Salvatore; Weiss, Rainer; Yam, William; Yu, H; Zucker, Michael E; Brown N. M.; ... Show more Show less
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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.
Date issued
2017-01Department
Massachusetts Institute of Technology. Department of Physics; Lincoln Laboratory; MIT Kavli Institute for Astrophysics and Space ResearchJournal
Classical and Quantum Gravity
Publisher
IOP Publishing
Citation
Abbott, B P et al. “Exploring the Sensitivity of Next Generation Gravitational Wave Detectors.” Classical and Quantum Gravity 34, 4 (January 2017): 044001© 2017 IOP Publishing Ltd
Version: Original manuscript
ISSN
0264-9381
1361-6382
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