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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3J9RMFP
Repositorysid.inpe.br/mtc-m21b/2015/04.07.16.47   (restricted access)
Last Update2015:04.07.16.48.14 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2015/04.07.16.47.40
Metadata Last Update2018:06.04.02.55.21 (UTC) administrator
DOI10.1088/1748-0221/10/03/P03001
ISSN1748-0221
Citation KeyPaulaFerrCarvAgui:2015:HiSeNi
TitleHigh sensitivity niobium parametric transducer for the Mario Schenberg gravitational wave detector
Year2015
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3415 KiB
2. Context
Author1 Paula, L. A. N.
2 Ferreira, Elvis Camilo
3 Carvalho, N. C.
4 Aguiar, Odylio Denys de
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ2A
Group1
2 AST-CEA-SPG-INPE-MCTI-GOV-BR
3
4 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Tecnológico de Aeronáutica (ITA)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 University of Western Australia
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 leandroifusp@yahoo.com
2 elvis.ferreira@inpe.br
3
4 odylio.aguiar@inpe.br
JournalJournal of Instrumentation
Volume10
History (UTC)2015-04-07 16:47:40 :: simone -> administrator ::
2018-06-04 02:55:21 :: administrator -> simone :: 2015
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsInstrument optimisation
resonant deterctors
modeling of microwave systems
AbstractParametric transducers can work below the quantum limit of sensitivity for resonant mass gravitational wave detectors. This makes them a promising alternative for electromechanical transductance for such detectors. These transducers consist of a reentrant superconducting niobium cavity coupled to a mass-spring system with three mechanical modes. These cavities have a central post responsible for creating a narrow axial gap between its top and the cavity wall, which is a resonant membrane. Their displacement sensitivity (df/dx) increases as the gap spacing decreases. However, this is not a linear relationship and the dimensioning of the cavity becomes critical if the gap is of the order of a few microns. In this paper, we describe how to obtain a gap spacing of ~ 3 μ m and also the development of parametric transducers that will be employed in the coming experimental runs of the Schenberg gravitational wave antenna. Mechanical thinning methods were performed followed by mechanical and electrical frequency measurements to tune the device to operate at the required frequencies. The main results present better frequency stability and an improvement of df/dx by one order of magnitude higher than the preceding models. These results will allow us to reach the quantum limit of detector sensitivity of ~ 10−22 Hz−1/2 in the near future, making it possible to search for gravitational waves around 3.2 kHz.
AreaCEA
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5. Allied materials
Linking8JMKD3MGP7W/3FMELKS
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3ETR8EH
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Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.26 2
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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