Exploring the sensitivity of next generation gravitational wave detectors

LIGO Scientific Collaboration

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

© 2017 IOP Publishing Ltd.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.
Original languageEnglish
Article number044001
JournalClassical and Quantum Gravity
Volume34
Issue number4
DOIs
Publication statusPublished - 24 Jan 2017
Externally publishedYes

Funding

LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement PHY-0757058. Advanced LIGO was built under award PHY- 0823459. This paper carries LIGO Document Number LIGO-P1600143.

FundersFunder number
California Institute of Technology and Massachusetts Institute of Technology
National Science FoundationPHY- 0823459, PHY-0757058, LIGO-P1600143
Directorate for Mathematical and Physical Sciences0757058, 0823459

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