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A cryogenic silicon interferometer for gravitational-wave detection

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dc.contributor.authorAdhikari, Rana X
dc.contributor.authorArai, Koji
dc.contributor.authorBrooks, AF
dc.contributor.authorWipf, C
dc.contributor.authorAguiar, O
dc.contributor.authorAltin, Paul
dc.contributor.authorBarr, B
dc.contributor.authorBarsotti, L
dc.contributor.authorBassiri, R
dc.contributor.authorBell, A
dc.contributor.authorBillingsley, G
dc.contributor.authorEichholz, Johannes
dc.contributor.authorKapasi, Disha
dc.contributor.authorMcClelland, David
dc.contributor.authorMcRae, Terry
dc.contributor.authorShaddock, Daniel
dc.contributor.authorSlagmolen, Bram
dc.contributor.authorWade, Andrew
dc.contributor.authorWard, Robert
dc.contributor.authorYap, Min Jet
dc.date.accessioned2022-02-03T22:52:54Z
dc.date.available2022-02-03T22:52:54Z
dc.date.issued2020
dc.date.updated2023-10-29T07:15:37Z
dc.description.abstractThe detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravitational wave astronomy, revealing a previously hidden side of the cosmos. To maximize the reach of the existing LIGO observatory facilities, we have designed a new instrument able to detect gravitational waves at distances 5 times further away than possible with Advanced LIGO, or at greater than 100 times the event rate. Observations with this new instrument will make possible dramatic steps toward understanding the physics of the nearby Universe, as well as observing the Universe out to cosmological distances by the detection of binary black hole coalescences. This article presents the instrument design and a quantitative analysis of the anticipated noise floor.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0264-9381en_AU
dc.identifier.urihttp://hdl.handle.net/1885/259052
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/11260..."The Accepted Version can be archived in a Non-Commercial Institutional Repository. 12 months embargo" from SHERPA/RoMEO site (as at 4/02/2022). This is an author-created, un-copyedited version of an article accepted for publication/published in [Classical and Quantum Gravity]. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://dx.doi.org/10.1088/1361-6382/ab9143en_AU
dc.publisherInstitute of Physics Publishing
dc.rights© 2020 IOP Publishing Ltd
dc.sourceClassical and Quantum Gravity
dc.subjectgravitational wave astronomy
dc.subjectinterferometry
dc.subjectcryogenic silicon
dc.subjectnext generation gravitational wave detection
dc.subjecttwo micron lasers
dc.subjectbinary black holes
dc.titleA cryogenic silicon interferometer for gravitational-wave detection
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue16en_AU
local.bibliographicCitation.lastpage40en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationAdhikari, Rana X, California Institute of Technologyen_AU
local.contributor.affiliationArai, Koji, California Institute of Technologyen_AU
local.contributor.affiliationBrooks, AF, LIGOen_AU
local.contributor.affiliationWipf, C, California Institute of Technologyen_AU
local.contributor.affiliationAguiar, O, Instituto Nacional de Pesquisas Espaciaisen_AU
local.contributor.affiliationAltin, Paul, College of Science, ANUen_AU
local.contributor.affiliationBarr, B, University of Glasgowen_AU
local.contributor.affiliationBarsotti, L, Massachusetts Institute of Technologyen_AU
local.contributor.affiliationBassiri, R, Stanford Universityen_AU
local.contributor.affiliationBell, A, University of Glasgowen_AU
local.contributor.affiliationBillingsley, G, California Institute of Technologyen_AU
local.contributor.affiliationEichholz, Johannes, College of Science, ANUen_AU
local.contributor.affiliationKapasi, Disha, Academic Portfolio, ANUen_AU
local.contributor.affiliationMcClelland, David, College of Science, ANUen_AU
local.contributor.affiliationMcRae, Terry, College of Science, ANUen_AU
local.contributor.affiliationShaddock, Daniel, College of Science, ANUen_AU
local.contributor.affiliationSlagmolen, Bram, College of Science, ANUen_AU
local.contributor.affiliationWade, Andrew, College of Science, ANUen_AU
local.contributor.affiliationWard, Robert, College of Science, ANUen_AU
local.contributor.affiliationYap, Min Jet, College of Science, ANUen_AU
local.contributor.authoruidAltin, Paul, u4103634en_AU
local.contributor.authoruidEichholz, Johannes, u1073016en_AU
local.contributor.authoruidKapasi, Disha, u6931556en_AU
local.contributor.authoruidMcClelland, David, u8802403en_AU
local.contributor.authoruidMcRae, Terry, u1008768en_AU
local.contributor.authoruidShaddock, Daniel, u9701638en_AU
local.contributor.authoruidSlagmolen, Bram, u9905035en_AU
local.contributor.authoruidWade, Andrew, u4311433en_AU
local.contributor.authoruidWard, Robert, u5088188en_AU
local.contributor.authoruidYap, Min Jet, u5021389en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020105 - General Relativity and Gravitational Wavesen_AU
local.identifier.absfor020102 - Astronomical and Space Instrumentationen_AU
local.identifier.absfor020604 - Quantum Opticsen_AU
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciencesen_AU
local.identifier.ariespublicationa383154xPUB14895en_AU
local.identifier.citationvolume37en_AU
local.identifier.doi10.1088/1361-6382/ab9143en_AU
local.identifier.scopusID2-s2.0-85089898054
local.identifier.thomsonIDWOS:000559743200001
local.publisher.urlhttp://iopscience.iop.org/0264-9381en_AU
local.type.statusAccepted Versionen_AU

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