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dc.contributor.authorBarsotti, Lisa
dc.contributor.authorEvans, Matthew J
dc.contributor.authorGras, Slawomir
dc.contributor.authorHall, E. D.
dc.contributor.authorKomori, Kentaro
dc.contributor.authorKuns, K.
dc.contributor.authorMansell, Georgia L.
dc.contributor.authorShoemaker, David H
dc.contributor.authorWeiss, Rainer
dc.date.accessioned2022-10-20T15:02:26Z
dc.date.available2021-09-20T18:22:19Z
dc.date.available2022-10-20T15:02:26Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/132426.2
dc.description.abstract© 2020 IOP Publishing Ltd. The 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.en_US
dc.language.isoen
dc.publisherIOP Publishingen_US
dc.relation.isversionof10.1088/1361-6382/ab9143en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleA cryogenic silicon interferometer for gravitational-wave detectionen_US
dc.typeArticleen_US
dc.contributor.departmentLIGO (Observatory : Massachusetts Institute of Technology)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalClassical and Quantum Gravityen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-10-21T17:05:03Z
dspace.orderedauthorsAdhikari, RX; Arai, K; Brooks, AF; Wipf, C; Aguiar, O; Altin, P; Barr, B; Barsotti, L; Bassiri, R; Bell, A; Billingsley, G; Birney, R; Blair, D; Bonilla, E; Briggs, J; Brown, DD; Byer, R; Cao, H; Constancio, M; Cooper, S; Corbitt, T; Coyne, D; Cumming, A; Daw, E; deRosa, R; Eddolls, G; Eichholz, J; Evans, M; Fejer, M; Ferreira, EC; Freise, A; Frolov, VV; Gras, S; Green, A; Grote, H; Gustafson, E; Hall, ED; Hammond, G; Harms, J; Harry, G; Haughian, K; Heinert, D; Heintze, M; Hellman, F; Hennig, J; Hennig, M; Hild, S; Hough, J; Johnson, W; Kamai, B; Kapasi, D; Komori, K; Koptsov, D; Korobko, M; Korth, WZ; Kuns, K; Lantz, B; Leavey, S; Magana-Sandoval, F; Mansell, G; Markosyan, A; Markowitz, A; Martin, I; Martin, R; Martynov, D; McClelland, DE; McGhee, G; McRae, T; Mills, J; Mitrofanov, V; Molina-Ruiz, M; Mow-Lowry, C; Munch, J; Murray, P; Ng, S; Okada, MA; Ottaway, DJ; Prokhorov, L; Quetschke, V; Reid, S; Reitze, D; Richardson, J; Robie, R; Romero-Shaw, I; Route, R; Rowan, S; Schnabel, R; Schneewind, M; Seifert, F; Shaddock, D; Shapiro, B; Shoemaker, D; Silva, AS; Slagmolen, B; Smith, J; Smith, N; Steinlechner, J; Strain, K; Taira, D; Tait, S; Tanner, D; Tornasi, Z; Torrie, C; Van Veggel, M; Vanheijningen, J; Veitch, P; Wade, A; Wallace, G; Ward, R; Weiss, R; Wessels, P; Willke, B; Yamamoto, H; Yap, MJ; Zhao, Cen_US
dspace.date.submission2020-10-21T17:05:06Z
mit.journal.volume37en_US
mit.journal.issue16en_US
mit.licenseOPEN_ACCESS_POLICY
mit.metadata.statusPublication Information Neededen_US


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