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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZGivnJVY/M2gD4
Repositóriosid.inpe.br/mtc-m16@80/2006/08.01.18.40   (acesso restrito)
Última Atualização2006:08.01.18.40.18 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m16@80/2006/08.01.18.40.19
Última Atualização dos Metadados2018:06.05.01.16.54 (UTC) administrator
Chave SecundáriaINPE-13922--PRE/9102
ISSN1742-6588
Chave de CitaçãoCostaAgui:2006:SiReMA
TítuloSimulated Response of the MARIO SCHENBERG Detector to Gravitational Wave Signals with Noise
Ano2006
Data de Acesso20 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho481 KiB
2. Contextualização
Autor1 Costa, César Augusto
2 Aguiar, Odylio Denys
Grupo1 DAS-INPE-MCT-BR
2 DAS-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
RevistaJournal of Physics: Conference Series
Volume32
Páginas18-22
Histórico (UTC)2006-08-01 18:40:19 :: simone -> administrator ::
2006-09-28 22:33:15 :: administrator -> simone ::
2006-12-12 17:01:29 :: simone -> administrator ::
2008-06-10 22:43:10 :: administrator -> simone ::
2008-07-23 17:02:41 :: simone -> administrator ::
2012-07-17 12:47:30 :: administrator -> banon :: 2006
2012-09-27 18:28:24 :: banon -> administrator :: 2006
2018-06-05 01:16:54 :: administrator -> marciana :: 2006
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThe Mario Schenberg gravitational wave detector has been constructed at its site in the Physics Institute of the University of Sao Paulo as programmed by the Brazilian Graviton Project under full financial support from FAPESP (the Sao Paulo State Foundation for Research Support). We are ready to do a first test run of the spherical antenna at 4.2 K with three parametric transducers and an initial target sensitivity of h ~ 10-21 Hz-½ in a 60 Hz bandwidth around 3.2 kHz. We have built a computer code for determining the source direction and the wave polarization (solution of the inverse problem) in real time acquisition for strong signal-to-noise ratio cases. The digital filter used is a simple bandpass filter. The ''data'' used for testing our code was simulated, it had both the source signal and detector noise. The detector noise includes the antenna thermal, back action, phase noise, series noise and thermal from transducer coupled masses. The simulated noise takes into account all these noise and the antenna-transducers coupling. The detector transfer function was calculated for a spherical antenna with six two-mode parametric transducers. Finally, we were able to check at what distance Schenberg would detected some known sources. Here we present the results of these simulations.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Simulated Response of...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo AlvoSimulated responses of the Mario.pdf
Grupo de Usuáriosadministrator
banon
simone
Visibilidadeshown
Detentor da CópiaSID/SCD
Política de Arquivamentodenypublisher denyfinaldraft12
Permissão de Leituradeny from all and allow from 150.163
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
6. Notas
NotasArtigo apresentado no: VI Edoardo Amaldi Conference on Gravitational Waves. Okinawa, Japan
Campos Vaziosalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn keywords label lineage mark mirrorrepository month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
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