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Frequency dependence of thermal noise in gram-scale cantilever flexures

dc.contributor.authorNguyen, Thanh
dc.contributor.authorMow-Lowry, Conor M
dc.contributor.authorSlagmolen, Bram
dc.contributor.authorMiller, John
dc.contributor.authorMullavey, Adam
dc.contributor.authorGossler, S
dc.contributor.authorAltin, Paul
dc.contributor.authorShaddock, Daniel
dc.contributor.authorMcClelland, David
dc.date.accessioned2018-11-29T22:55:28Z
dc.date.available2018-11-29T22:55:28Z
dc.date.issued2015
dc.date.updated2018-11-29T08:06:30Z
dc.description.abstractWe present measurements of the frequency dependence of thermal noise in aluminum and niobium flexures. Our measurements cover the audio-frequency band from 10 Hz to 10 kHz, which is of particular relevance to ground-based interferometric gravitational wave detectors, and span up to an order of magnitude above and below the fundamental flexure resonances. Results from two flexures are well explained by a simple model in which both structural and thermoelastic loss play a role. The ability of such a model to explain this interplay is important for investigations of quantum-radiation-pressure noise and the standard quantum limit. Furthermore, measurements on a third flexure provide evidence that surface damage can affect the frequency dependence of thermal noise in addition to reducing the quality factor, a result which will aid the understanding of how aging effects impact on thermal noise behavior.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1885/153166
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D-Particles, Fields, Gravitation and Cosmology
dc.titleFrequency dependence of thermal noise in gram-scale cantilever flexures
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue11
local.bibliographicCitation.lastpage7
local.bibliographicCitation.startpage112004/1
local.contributor.affiliationNguyen, Thanh, College of Science, ANU
local.contributor.affiliationMow-Lowry, Conor M, The University of Birmingham
local.contributor.affiliationSlagmolen, Bram, College of Science, ANU
local.contributor.affiliationMiller, John, LIGO
local.contributor.affiliationMullavey, Adam, Louisiana State University
local.contributor.affiliationGossler, S, University of Hannover
local.contributor.affiliationAltin, Paul, College of Science, ANU
local.contributor.affiliationShaddock, Daniel, College of Science, ANU
local.contributor.affiliationMcClelland, David, College of Science, ANU
local.contributor.authoruidNguyen, Thanh, u4216762
local.contributor.authoruidSlagmolen, Bram, u9905035
local.contributor.authoruidAltin, Paul, u4103634
local.contributor.authoruidShaddock, Daniel, u9701638
local.contributor.authoruidMcClelland, David, u8802403
local.description.notesImported from ARIES
local.identifier.absfor020502 - Lasers and Quantum Electronics
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB8513
local.identifier.citationvolume92
local.identifier.doi10.1103/PhysRevD.92.112004
local.identifier.scopusID2-s2.0-84952332666
local.identifier.thomsonID000366501700002
local.type.statusPublished Version

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