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dc.contributor.authorMiao, Haixing
dc.contributor.authorSmith, Nicolas D.
dc.contributor.authorEvans, Matthew J
dc.date.accessioned2020-05-04T17:54:03Z
dc.date.available2020-05-04T17:54:03Z
dc.date.issued2019-03
dc.date.submitted2019-01
dc.identifier.issn2160-3308
dc.identifier.urihttps://hdl.handle.net/1721.1/124998
dc.description.abstractWe derive a quantum limit to the sensitivity of laser interferometric gravitational-wave detectors from optical-loss-induced dissipation, analogous to the sensitivity limit from the mechanical dissipation. It applies universally to different interferometer configurations and cannot be surpassed unless the optical properties of the interferometer are improved. This result provides an answer to the long-standing question of how far we can push the detector sensitivity given the state-of-the-art optics. Subject Areas: Gravitation, Optics, Quantum Physicsen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevX.9.011053en_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0en_US
dc.sourceAmerican Physical Societyen_US
dc.titleQuantum Limit for Laser Interferometric Gravitational-Wave Detectors from Optical Dissipationen_US
dc.typeArticleen_US
dc.identifier.citationMiao, Haixing, et al. “Quantum Limit for Laser Interferometric Gravitational-Wave Detectors from Optical Dissipation.” Physical Review X 9, 1 (March 2019): 011053 © 2019 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.relation.journalPhysical Review Xen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-03-26T18:00:09Z
dc.language.rfc3066en
dspace.embargo.termsNen_US
dspace.date.submission2019-04-04T11:56:30Z
mit.journal.volume9en_US
mit.journal.issue1en_US
mit.licensePUBLISHER_CCen_US


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