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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3LKDDEE
Repositorysid.inpe.br/mtc-m21b/2016/05.02.13.23   (restricted access)
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Metadata Repositorysid.inpe.br/mtc-m21b/2016/05.02.13.23.23
Metadata Last Update2018:06.04.02.40.44 (UTC) administrator
DOI10.1007/s10714-016-2038-1
ISSN0001-7701
Citation KeyCedeñoMontañaAraú:2016:GrRaPo
TitleGravitational radiation by point particle eccentric binary systems in the linearised characteristic formulation of general relativity
Year2016
MonthApr.
Access Date2024, June 21
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size523 KiB
2. Context
Author1 Cedeño Montaña, Carlos Eduardo
2 Araújo, José Carlos Neves de
Resume Identifier1
2 8JMKD3MGP5W/3C9JHGK
Group1 AST-CEA-SPG-INPE-MCTI-GOV-BR
2 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 eduardo.montana@inpe.br
2 jcarlos.dearaujo@inpe.br
JournalGeneral Relativity and Gravitation
Volume48
Number4
Pages45
Secondary MarkB1_QUÍMICA B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_ASTRONOMIA_/_FÍSICA
History (UTC)2016-05-02 13:23:23 :: simone -> administrator ::
2018-06-04 02:40:44 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGeneral relativity
Characteristic formulation
Linear regime
Approximation methods
AbstractWe study a binary system composed of point particles of unequal masses in eccentric orbits in the linear regime of the characteristic formulation of general relativity, generalising a previous study found in the literature in which a system of equal masses in circular orbits is considered. We also show that the boundary conditions on the time-like world tubes generated by the orbits of the particles can be extended beyond circular orbits. Concerning the power lost by the emission of gravitational waves, it is directly obtained from the Bondi's News function. It is worth stressing that our results are completely consistent, because we obtain the same result for the power derived by Peters and Mathews, in a different approach, in their seminal paper of 1963. In addition, the present study constitutes a powerful tool to construct extraction schemes in the characteristic formalism to obtain the gravitational radiation produced by binary systems during the inspiralling phase.
AreaCEA
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6. Notes
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