Adelaide Research & Scholarship
Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/116533
| Citations | ||
| Scopus | Web of Science® | Altmetric |
|---|---|---|
|
?
|
?
|
|
| Type: | Journal article |
| Title: | Exploring the sensitivity of next generation gravitational wave detectors |
| Author: | Abbott, B. Abbott, R. Abbott, T. Abernathy, M. Ackley, K. Adams, C. Addesso, P. Adhikari, R. Adya, V. Affeldt, C. Aggarwal, N. Aguiar, O. Ain, A. Ajith, P. Allen, B. Altin, P. Anderson, S. Anderson, W. Arai, K. Araya, M. et al. |
| Citation: | Classical and Quantum Gravity, 2017; 34(4):044001-1-044001-18 |
| Publisher: | IOP Publishing Ltd |
| Issue Date: | 2017 |
| ISSN: | 0264-9381 1361-6382 |
| Statement of Responsibility: | B P Abbott ... W Kim ... E J King ... J Munch ... D J Ottaway ... P J Veitch ... et al. |
| 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 gravitationalwave 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. |
| Keywords: | Gravitational waves; cosmic explorer; LIGO |
| Rights: | © 2017 IOP Publishing Ltd |
| DOI: | 10.1088/1361-6382/aa51f4 |
| Grant ID: | PHY-0823459 |
| Published version: | http://dx.doi.org/10.1088/1361-6382/aa51f4 |
| Appears in Collections: | Aurora harvest 3 IPAS publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| hdl_116533.pdf | Accepted version | 1.64 MB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.