Exploring the sensitivity of next generation gravitational wave detectors

Abbott, B. P.; Davies, G. S.; LIGO Scientific Collaboration

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.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.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.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