Exploring the sensitivity of next generation gravitational wave detectors

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dc.contributor.authorAbbott, B.
dc.contributor.authorAbbott, R.
dc.contributor.authorAbbott, T.
dc.contributor.authorAbernathy, M.
dc.contributor.authorAckley, K.
dc.contributor.authorAdams, C.
dc.contributor.authorAddesso, P.
dc.contributor.authorAdhikari, R.
dc.contributor.authorAdya, V.
dc.contributor.authorAffeldt, C.
dc.contributor.authorAggarwal, N.
dc.contributor.authorAguiar, O.
dc.contributor.authorAin, A.
dc.contributor.authorAjith, P.
dc.contributor.authorAllen, B.
dc.contributor.authorAltin, P.
dc.contributor.authorAnderson, S.
dc.contributor.authorAnderson, W.
dc.contributor.authorArai, K.
dc.contributor.authorAraya, M.
dc.contributor.authoret al.
dc.date.issued2017
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 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.
dc.description.statementofresponsibilityB P Abbott ... W Kim ... E J King ... J Munch ... D J Ottaway ... P J Veitch ... et al.
dc.identifier.citationClassical and Quantum Gravity, 2017; 34(4):044001-1-044001-18
dc.identifier.doi10.1088/1361-6382/aa51f4
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.orcidBrown, D. [0000-0001-7851-3939]
dc.identifier.urihttp://hdl.handle.net/2440/116533
dc.language.isoen
dc.publisherIOP Publishing Ltd
dc.relation.grantPHY-0823459
dc.rights© 2017 IOP Publishing Ltd
dc.source.urihttps://doi.org/10.1088/1361-6382/aa51f4
dc.subjectGravitational waves; cosmic explorer; LIGO
dc.titleExploring the sensitivity of next generation gravitational wave detectors
dc.typeJournal article
pubs.publication-statusPublished

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