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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/4873UFH
Repositorysid.inpe.br/plutao/2022/12.12.17.23.48
Last Update2022:12.16.10.46.12 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2022/12.12.17.23.49
Metadata Last Update2023:01.03.16.52.56 (UTC) administrator
DOI10.1142/9789811258251_0226
ISBN9789811258244
Labellattes: 6217296674061205 1 AraujoCoelLadiCost:2022:GrWaPu
Citation KeyAraújoCoelLadiCost:2022:GrWaPu
TitleGravitational waves from pulsars due to their magnetic ellipticity
Year2022
Access Date2024, May 12
Secondary TypePRE CI
Number of Files1
Size324 KiB
2. Context
Author1 Araújo, José Carlos Neves de
2 Coelho, Jaziel G.
3 Ladislau, Samantha Monaliza
4 Costa, Cesar Augusto
Resume Identifier1 8JMKD3MGP5W/3C9JHGK
Group1 DIAST-CGCE-INPE-MCTI-GOV-BR
2
3 DIAST-CGCE-INPE-MCTI-GOV-BR
4 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Tecnológica Federal do Paraná (UTFPR)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jcarlos.dearaujo@inpe.br
2
3 samantha.ladislau@inpe.br
4 cesar.costa@inpe.br
Conference NameMG15 Meeting on General Relativity
Conference LocationUniversity of Rome La Sapienza
Date2018
Pages1539
Book TitleProceedings
Tertiary TypePaper
History (UTC)2022-12-16 10:46:14 :: lattes -> administrator :: 2022
2022-12-17 09:22:53 :: administrator -> lattes :: 2022
2022-12-19 19:10:42 :: lattes -> administrator :: 2022
2023-01-03 16:52:56 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsPulsars
Estrela de Neutrons
AbstractWe discuss some aspects of de Araujo, Coelho and Costa 1,2 concerning the role of a time dependent magnetic ellipticity on the pulsars braking indices and on the putative gravitational waves (GWs) these objects can emit. Since only nine of more than 2000 known pulsars have accurately measured braking indices, it is of interest to extend this study to all known pulsars, in particular as regards GW generation. In summary, our results show a pessimistic prospect for the detection of GWs generated by these pulsars, even for advanced detectors such as aLIGO and AdVirgo, and the planned Einstein Telescope, would not be able to detect these pulsar, if the ellipticity has magnetic origin.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Gravitational waves from...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W/4873UFH
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W/4873UFH
Languageen
Target File1906.00774.pdf
User Grouplattes
Reader Groupadministrator
lattes
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 2
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
NotesSetores de Atividade: Pesquisa e desenvolvimento científico.
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination e-mailaddress edition editor format issn lineage mark mirrorrepository nextedition numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume
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