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Mechanical characterisation of the TorPeDO: a low frequency gravitational force sensor

McManus, David; Forsyth, Perry; Yap, Min Jet; Ward, Robert; Shaddock, Daniel; McClelland, David; Slagmolen, Bram

Description

Newtonian noise is likely to be a future challenge at low frequencies for Advanced LIGO and other second generation gravitational wave detectors. We present the TorPeDO system: a dual torsion pendulum sensor designed to measure local gravitational forces to high precision. Gravitational forces induce a differential rotation between the two torsion beams, which is measured with an optical read-out. Both torsion pendulums have a common suspension point, tunable centre of mass, and resonant...[Show more]

dc.contributor.authorMcManus, David
dc.contributor.authorForsyth, Perry
dc.contributor.authorYap, Min Jet
dc.contributor.authorWard, Robert
dc.contributor.authorShaddock, Daniel
dc.contributor.authorMcClelland, David
dc.contributor.authorSlagmolen, Bram
dc.date.accessioned2021-08-06T00:14:17Z
dc.identifier.issn0264-9381
dc.identifier.urihttp://hdl.handle.net/1885/243237
dc.description.abstractNewtonian noise is likely to be a future challenge at low frequencies for Advanced LIGO and other second generation gravitational wave detectors. We present the TorPeDO system: a dual torsion pendulum sensor designed to measure local gravitational forces to high precision. Gravitational forces induce a differential rotation between the two torsion beams, which is measured with an optical read-out. Both torsion pendulums have a common suspension point, tunable centre of mass, and resonant frequency. This produces a high level of mechanical common mode noise cancellation. We report on a controls prototype of the TorPeDO system, presenting the frequency response and tuning range of both pendulums. A noise budget and mechanical cross-coupling model for this system are also presented. We demonstrate frequency tuning of the two torsion pendulums to a difference of 4.3 μHz.
dc.description.sponsorshipBS, RW and DM would like to acknowledge support from the Australian Research Council grant FT130100329 and DP160100760. This paper has been assigned LIGO document number P1700004.
dc.format.mimetypeapplication/pdf
dc.language.isoen_AU
dc.publisherInstitute of Physics Publishing
dc.rights© 2017 IOP Publishing Ltd
dc.sourceClassical and Quantum Gravity
dc.subjectgravitational waves
dc.subjectnewtonian noise
dc.subjecttorsion pendulum
dc.subjectoptical sensing
dc.subjectgravimeter
dc.titleMechanical characterisation of the TorPeDO: a low frequency gravitational force sensor
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume34
dc.date.issued2017
local.identifier.absfor010505 - Mathematical Aspects of Quantum and Conformal Field Theory, Quantum Gravity and String Theory
local.identifier.ariespublicationa383154xPUB7067
local.publisher.urlhttp://iopscience.iop.org/0264-9381
local.type.statusPublished Version
local.contributor.affiliationMcManus, David, College of Science, ANU
local.contributor.affiliationForsyth, Perry, College of Science, ANU
local.contributor.affiliationYap, Min Jet, College of Science, ANU
local.contributor.affiliationWard, Robert, College of Science, ANU
local.contributor.affiliationShaddock, Daniel, College of Science, ANU
local.contributor.affiliationMcClelland, David, College of Science, ANU
local.contributor.affiliationSlagmolen, Bram, College of Science, ANU
local.description.embargo2099-12-31
dc.relationhttp://purl.org/au-research/grants/arc/FT130100329
dc.relationhttp://purl.org/au-research/grants/arc/DP160100760
local.bibliographicCitation.issue13
local.bibliographicCitation.startpage1
local.bibliographicCitation.lastpage12
local.identifier.doi10.1088/1361-6382/aa7103
dc.date.updated2020-11-23T10:48:31Z
local.identifier.scopusID2-s2.0-85021075145
local.identifier.thomsonID000403049400002
CollectionsANU Research Publications

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