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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PJDA25
Repositorysid.inpe.br/mtc-m21b/2017/09.06.14.29   (restricted access)
Last Update2017:09.06.14.29.12 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/09.06.14.29.12
Metadata Last Update2018:06.04.02.27.50 (UTC) administrator
DOI10.1088/1361-6382/aa7fff
ISSN0264-9381
Citation KeyCarvalhoBourTobaAgui:2017:SeChPa
TitleSensitivity characterisation of a parametric transducer for gravitational wave detection through optical spring effect
Year2017
MonthJuly
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1162 KiB
2. Context
Author1 Carvalho, Natalia C.
2 Bourhill, J.
3 Tobar, M. E.
4 Aguiar, Odylio Denys de
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ2A
Group1
2
3
4 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 University of Western Australia
2 University of Western Australia
3 University of Western Australia
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 nataliaccar@gmail.com
2
3
4 odylio.aguiar@inpe.br
JournalClassical and Quantum Gravity
Volume34
Number17
PagesArticle number 175001
Secondary MarkA1_ENGENHARIAS_I A2_INTERDISCIPLINAR A2_ASTRONOMIA_/_FÍSICA B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_ENGENHARIAS_IV B2_ENSINO
History (UTC)2017-09-06 14:29:12 :: simone -> administrator ::
2017-09-06 14:29:13 :: administrator -> simone :: 2017
2017-09-06 14:29:36 :: simone -> administrator :: 2017
2018-06-04 02:27:50 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitational waves
gravitational wave detectors
optomechanics
microwave
AbstractWe present the characterisation of the most recent parametric transducers designed to enhance the Mario Schenberg gravitational wave detector sensitivity. The transducer is composed of a microwave re-entrant cavity that attaches to the gravitational wave antenna via a rigid spring. It functions as a three-mode mass-spring system; motion of the spherical antenna couples to a 50 μm thick membrane, which converts its mechanical motion into a frequency shift of the cavity resonance. Through the optical spring effect, the microwave transducer frequency-displacement sensitivity was measured to be 726 MHz μm-1 at 4 K. The spherical antenna detection sensitivity is determined analytically using the transducer amplification gain and equivalent displacement noise in the test setup, which are 5.5 × 1011 V m-1 and 1.8 × 1019 m √Hz-1, respectively.
AreaCEA
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4. Conditions of access and use
Languageen
Target FileCarvalho_2017_Class._Quantum_Grav._34_175001.pdf
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Visibilityshown
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.26 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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