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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3FCL3GB
Repositorysid.inpe.br/plutao/2013/12.12.15.15   (restricted access)
Last Update2014:01.16.16.04.27 (UTC) administrator
Metadata Repositorysid.inpe.br/plutao/2013/12.12.15.15.49
Metadata Last Update2018:06.04.23.39.13 (UTC) administrator
DOI10.1142/S0217732313501745
ISSN0217-7323
Labellattes: 6217296674061205 2 EvangelistaArau:2013:NEMECA
Citation KeyEvangelistaArau:2013:NeMeCa
TitleA new method to calculate the stochastic background of gravitational waves generated by compact binaries
Year2013
Access Date2024, June 21
Secondary TypePRE PI
Number of Files1
Size203 KiB
2. Context
Author1 Evangelista, Edgard F. D.
2 Araujo, Jose Carlos Neves de
Resume Identifier1
2 8JMKD3MGP5W/3C9JHGK
Group1
2 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 jcarlos.dearaujo@inpe.br
e-Mail Addressjcarlos.dearaujo@inpe.br
JournalModern Physics Letters A
Volume28
Number38
Pages1350174
Secondary MarkB1 B3 B3 B3
History (UTC)2013-12-12 15:15:49 :: lattes -> administrator ::
2018-06-04 23:39:13 :: administrator -> marcelo.pazos@inpe.br :: 2013
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsOndas Gravitacionais
Estrelas de Neutrons
Fundos Cosmológicos de Ondas Gravitacionais
Gravitational waves
stochastic background
double neutron stars
AbstractIn the study of gravitational waves (GWs), the stochastic background generated by compact binary systems are among the most important kinds of signals. The reason for such an importance has to do with their probable detection by the interferometric detectors [such as the Advanced LIGO (ALIGO) and Einstein Telescope (ET)] in the near future. In this paper we are concerned with, in particular, the stochastic background of GWs generated by double neutron star (DNS) systems in circular orbits during their periodic and quasi-periodic phases. Our aim here is to describe a new method to calculate such spectra, which is based on an analogy with a problem of Statistical Mechanics. Besides, an important characteristic of our method is to consider the time evolution of the orbital parameters.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A new method...
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Languageen
User Grouplattes
marcelo.pazos@inpe.br
Reader Groupadministrator
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Update Permissionnot transferred
5. Allied materials
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 3
DisseminationWEBSCI; PORTALCAPES.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
NotesSetores de Atividade: Pesquisa e desenvolvimento científico.
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
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e-Mail (login)marcelo.pazos@inpe.br
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