Área de identificação | |
Tipo de Referência | Material Audiovisual (Audiovisual Material) |
Site | mtc-m16d.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP7W/3958U4B |
Repositório | sid.inpe.br/mtc-m19/2011/02.04.14.24.36 |
Metadados | sid.inpe.br/mtc-m19/2011/02.04.14.24.37 |
Última Atualização dos Metadados | 2018:06.05.04.35.26 administrator |
Chave Secundária | INPE--MAO/ |
Chave de Citação | EvangelistaAraú:2010:StBaGr |
Título | Stochastic background of gravitational waves generated by compact binary systems  |
Formato | On-line |
Ano | 2010 |
Data de Acesso | 04 mar. 2021 |
Área de contextualização | |
Autor | 1 Evangelista, Edgard de Freitas Diniz 2 Araújo, José Carlos Neves de |
Grupo | 1 DAS-CEA-INPE-MCT-BR 2 DAS-CEA-INPE-MCT-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
Nome do Evento | Workshop da Pós-Graduação, (DAS/INPE). |
Localização do Evento | Sao José dos Campos |
Data | 17 - 18 Nov. 2010 |
Editora (Publisher) | Instituto Nacional de Pesquisas Espaciais |
Cidade da Editora | São José dos Campos |
Histórico | 2011-02-04 14:37:54 :: marciana -> administrator :: 2010 2018-06-05 04:35:26 :: administrator -> marciana :: 2010 |
Área de conteúdo e estrutura | |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Resumo | Binary Systems are the the most studied sources of gravitational radiation, both theoretically and observationally. Theoretically, the mechanisms of emission and the behaviuor of the orbital parameters are well known and can be written in analytic form in several cases, which is a great advantage in terms of computational work; observationally, even though gravitational waves have not been detected yet, the strongest indication of the its existence have arisen from the observation of binary systems, more specifically the Hulse-Taylor binary pulsar. When one begins to detect gravitational radiation, one of the observed pattern of the signals will probably be of stochastic background nature because there will be a superposition of the signals emited by a plenty of sources around the Universe. So, our task here is to develop a method for summing the gravitational waves emited by cosmological binary compact systems in order to find out the shape of the spectra, that is, we will develop a method for obtaining the stochastic background generated by these systems. We use here an analogy with a problem of statistical mechanics in order to perform this sum, besides taking into account the temporal variation of the orbital parameters of the systems.. |
Area | CEA |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
Área de condições de acesso e uso | |
Idioma | pt |
Grupo de Usuários | marciana |
Visibilidade | shown |
Permissão de Leitura | allow from all |
Área de fontes relacionadas | |
Repositório Espelho | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH |
Acervo Hospedeiro | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
Área de notas | |
Campos Vazios | archivingpolicy archivist booktitle callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress electronicmailaddress isbn issn keywords label lineage mark nextedition notes numberoffiles numberofslides orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder secondarydate secondarymark secondarytype session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
Área de controle da descrição | |
e-Mail (login) | marciana |
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