Exploring the sensitivity of next generation gravitational wave detectors
dc.contributor.author | Abbott, B. P. | |
dc.contributor.author | Davies, G. S. | |
dc.contributor.author | LIGO Scientific Collaboration | |
dc.date.accessioned | 2017-04-05T15:12:31Z | |
dc.date.available | 2017-04-05T15:12:31Z | |
dc.date.issued | 2017-01-24 | |
dc.description.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. | en_UK |
dc.identifier.citation | Abbott, BP., et al., (LIGO Scientific Collaboration). (2017) Exploring the sensitivity of next generation gravitational wave detectors. Classical and Quantum Gravity, Volume 34, Issue 4, February 2017, Article number 044001 | en_UK |
dc.identifier.uri | http://dspace.lib.cranfield.ac.uk/handle/1826/11727 | |
dc.identifier.uri | http://dx.doi.org/10.1088/1361-6382/aa51f4 | |
dc.publisher | Institute of Physics | en_UK |
dc.rights | © 2017 Institute of Physics. This is the publisher Version of Record Manuscript. Please refer to any applicable publisher terms of use. | |
dc.title | Exploring the sensitivity of next generation gravitational wave detectors | en_UK |
dc.type | Article | en_UK |
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