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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3P8SECKy/CBhav
Repositorysid.inpe.br/jeferson/2004/06.29.10.54   (restricted access)
Last Update2006:06.14.04.04.02 (UTC) administrator
Metadata Repositorysid.inpe.br/jeferson/2004/06.29.10.54.24
Metadata Last Update2018:06.04.04.12.52 (UTC) administrator
Secondary KeyINPE-10786-PRE/6243
ISBN/ISSN0264-938
ISSN0264-9381
Citation KeyFrajucaLeAnAgMaMa:2004:NoMoBr
TitleA noise model for the Brazilian gravitational wave detector "Mario Schenberg"
Year2004
Secondary Date20040212
MonthMar.
Access Date2024, May 19
Secondary TypePRE PI
Number of Files1
Size72 KiB
2. Context
Author1 Frajuca, Carlos
2 Leite, Ribeiro Kilder
3 Andrade, Luiz A
4 Aguiar, Odylio Denys de
5 Magalhães, Nadja Simão
6 Marino Jr, Rubens de Melo
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ2A
Group1 DAS-INPE-MCT-BR
Affiliation1 Centro Federal de Educacao Tecnologica de Sao Paulo
2 Divisao de Astrofisica - Instituto Nacional de Pesquisas Espaciais
3 Instituto Tecnologica de Aeronautica - Departamento de Física
e-Mail Addressfrajuca@cefetsp.br
JournalClassical and Quantum Gravity
Volume21
Number5
PagesS1107 - S1111
History (UTC)2006-01-18 17:48:37 :: marciana -> administrator ::
2007-03-05 21:29:46 :: administrator -> marciana ::
2008-05-02 16:20:25 :: marciana -> administrator ::
2018-06-04 04:12:52 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsparametric transducer
antena
radiation
Abstract"Mario Schenberg" is a spherical resonant-mass gravitational wave (GW) detector that will be part of a GW detection array of three detectors. The other two will be built in Italy and in The Netherlands. Their resonant frequencies will be around 3.2 kHz with a bandwidth of about 200 Hz. This range of frequencies is new in a field where the typical frequencies lay below 1 kHz, making the development of the mechanical system much more complex. In this work, a noise model of the detector is presented, where all main sources of noise were taken into account. The final goal is to calculate the expected sensitivity of the detector, analysing which parameters must be changed to improve this.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A noise model...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileA noise model for the Brazilian gw detector.pdf
User Groupadministrator
marciana
valdirene
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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