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1. Identity statement
Reference TypeSlides (Audiovisual Material)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3958U4B
Repositorysid.inpe.br/mtc-m19/2011/02.04.14.24.36
Metadata Repositorysid.inpe.br/mtc-m19/2011/02.04.14.24.37
Metadata Last Update2018:06.05.04.35.26 (UTC) administrator
Secondary KeyINPE--MAO/
Citation KeyEvangelistaAraú:2010:StBaGr
TitleStochastic background of gravitational waves generated by compact binary systems
FormatOn-line
Year2010
Access Date2024, Mar. 29
2. Context
Author1 Evangelista, Edgard de Freitas Diniz
2 Araújo, José Carlos Neves de
Group1 DAS-CEA-INPE-MCT-BR
2 DAS-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference NameWorkshop da Pós-Graduação, (DAS/INPE).
Conference LocationSao José dos Campos
Date17 - 18 Nov. 2010
PublisherInstituto Nacional de Pesquisas Espaciais
Publisher CitySão José dos Campos
History (UTC)2011-02-04 14:37:54 :: marciana -> administrator :: 2010
2018-06-05 04:35:26 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractBinary 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..
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Stochastic background of...
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4. Conditions of access and use
Languagept
User Groupmarciana
Visibilityshown
Read Permissionallow from all
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy 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 schedulinginformation secondarydate secondarymark secondarytype session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Description control
e-Mail (login)marciana
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