Exploring the sensitivity of next generation gravitational wave detectors
Name
1607.08697.pdf
Size
1.31 MB
Format
Adobe PDF
Checksum (MD5)
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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
Date Issued
January 2017
Journal
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
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.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Lincoln Laboratory
MIT Kavli Institute for Astrophysics and Space Research
Terms of Use
Creative Commons Attribution-Noncommercial-Share Alike
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1088/1361-6382/AA51F4
