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dc.date.accessioned2021-09-20T18:22:19Z
dc.date.available2021-09-20T18:22:19Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/132426
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.
dc.language.isoen
dc.publisherIOP Publishing
dc.relation.isversionof10.1088/1361-6382/ab9143
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.sourcearXiv
dc.titleA cryogenic silicon interferometer for gravitational-wave detection
dc.typeArticle
dc.relation.journalClassical and Quantum Gravity
dc.eprint.versionAuthor's final manuscript
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
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, C
dspace.date.submission2020-10-21T17:05:06Z
mit.journal.volume37
mit.journal.issue16
mit.licenseOPEN_ACCESS_POLICY
mit.metadata.statusAuthority Work and Publication Information Needed


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