Exploring the sensitivity of next generation gravitational wave detectors

dc.contributor.authorAbbott, B. P.
dc.contributor.authorDavies, G. S.
dc.contributor.authorLIGO Scientific Collaboration
dc.date.accessioned2017-04-05T15:12:31Z
dc.date.available2017-04-05T15:12:31Z
dc.date.issued2017-01-24
dc.description.abstractThe 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.citationAbbott, 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 044001en_UK
dc.identifier.urihttp://dspace.lib.cranfield.ac.uk/handle/1826/11727
dc.identifier.urihttp://dx.doi.org/10.1088/1361-6382/aa51f4
dc.publisherInstitute of Physicsen_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.titleExploring the sensitivity of next generation gravitational wave detectorsen_UK
dc.typeArticleen_UK

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