Skip navigation
Skip navigation

Exploring the sensitivity of next generation gravitational wave detectors

Abbott, B P; Abbott, R; Abbott, T D; Abernathy, M R; Ackley, K; Adams, C; Addesso, P; Adhikari, Rana X; Affeldt, C; Adya, V; Altin, Paul; Chow, Jong; Mansell, Georgia; McClelland, David; McManus, David; McRae, Terry; Nguyen, Thanh; Rabeling, David; Scott, Susan M.; Shaddock, Daniel; Slagmolen, Bram; Wade, Andrew; Ward, Robert

Description

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.

CollectionsANU Research Publications
Date published: 2017
Type: Journal article
URI: http://hdl.handle.net/1885/303911
Source: Classical and Quantum Gravity
DOI: 10.1088/1361-6382/aa51f4

Download

File Description SizeFormat Image
Abbott_2017_Class._Quantum_Grav._34_044001.pdf2.2 MBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  17 November 2022/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator