1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZ3P8SECKy/CBhav |
Repository | sid.inpe.br/jeferson/2004/06.29.10.54 (restricted access) |
Last Update | 2006:06.14.04.04.02 (UTC) administrator |
Metadata Repository | sid.inpe.br/jeferson/2004/06.29.10.54.24 |
Metadata Last Update | 2018:06.04.04.12.52 (UTC) administrator |
Secondary Key | INPE-10786-PRE/6243 |
ISBN/ISSN | 0264-938 |
ISSN | 0264-9381 |
Citation Key | FrajucaLeAnAgMaMa:2004:NoMoBr |
Title | A noise model for the Brazilian gravitational wave detector "Mario Schenberg" |
Year | 2004 |
Secondary Date | 20040212 |
Month | Mar. |
Access Date | 2024, May 19 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 72 KiB |
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2. Context | |
Author | 1 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 Identifier | 1 2 3 4 8JMKD3MGP5W/3C9JJ2A |
Group | 1 DAS-INPE-MCT-BR |
Affiliation | 1 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 Address | frajuca@cefetsp.br |
Journal | Classical and Quantum Gravity |
Volume | 21 |
Number | 5 |
Pages | S1107 - 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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Keywords | parametric 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A noise model... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | A noise model for the Brazilian gw detector.pdf |
User Group | administrator marciana valdirene |
Visibility | shown |
Copy Holder | SID/SCD |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
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6. Notes | |
Empty Fields | alternatejournal 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 |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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