Journal article
Exploring the sensitivity of next generation gravitational wave detectors
BP Abbott, R Abbott, TD Abbott, MR Abernathy, K Ackley, C Adams, P Addesso, RX Adhikari, VB Adya, C Affeldt, N Aggarwal, OD Aguiar, A Ain, P Ajith, B Allen, PA Altin, SB Anderson, WG Anderson, K Arai, MC Araya Show all
Classical and Quantum Gravity | Published : 2017
Open access
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.
Grants
Awarded by National Science Foundation
Funding Acknowledgements
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.