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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3MPPDBE
Repositorysid.inpe.br/mtc-m21b/2016/11.11.12.20   (restricted access)
Last Update2016:11.11.12.20.11 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2016/11.11.12.20.11
Metadata Last Update2018:06.04.02.41.14 (UTC) administrator
DOI10.1088/1475-7516/2016/07/023
ISSN1475-7516
Citation KeyAraújoCoelCost:2016:GrWaEm
TitleGravitational wave emission by the high braking index pulsar PSR J1640-4631
Year2016
MonthJuly
Access Date2024, June 21
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size625 KiB
2. Context
Author1 Araújo, José Carlos Neves de
2 Coelho, Jaziel Goulart
3 Costa, César Augusto
Resume Identifier1 8JMKD3MGP5W/3C9JHGK
Group1 DAS-CEA-INPE-MCTI-GOV-BR
2 AST-CEA-SPG-INPE-MCTI-GOV-BR
3 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jcarlos.dearaujo@inpe.br
2 jaziel.coelho@inpe.br
3 cesar.costa@inpe.br
JournalJournal of Cosmology and Astroparticle Physics
Volume7
Pages023
Secondary MarkA1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA B1_GEOCIÊNCIAS
History (UTC)2016-11-11 12:20:11 :: simone -> administrator ::
2016-11-11 12:20:11 :: administrator -> simone :: 2016
2016-11-11 12:20:38 :: simone -> administrator :: 2016
2016-11-14 05:25:45 :: administrator -> simone :: 2016
2016-12-21 12:03:34 :: simone -> administrator :: 2016
2018-06-04 02:41:14 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitational waves / sources
neutron stars
AbstractRecently, a braking index for the pulsar PSR J1640-4631 has been measured. With a braking index of n = 3.15 +/- 0.03, this pulsar has the highest braking index ever measured. As it is well known, a pure magnetic dipole brake yields n = 3, whereas a pure gravitational wave (GW) brake yields n = 5. Therefore, each of these mechanisms alone can not account for the braking index found for PSR J1640-4631. Here we consider in detail that such a braking index could be accounted for if the spindown model combines magnetic dipole and GW brakes. Then, we briefly discuss the detectability of this pulsar by aLIGO and the planned Einstein Telescope. In particular, we show that the amplitude of the GW that comes from our model is around a factor four lower than the amplitude modeled exclusively by GW energy loss. Another interesting outcome of our modeling is that it is possible to obtain the ellipticity from the braking index and other pulsar parameters.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Gravitational wave emission...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > AST > Gravitational wave emission...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
Languageen
Target Filearaujo_gravitational.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3F2NE4L
Citing Item Listsid.inpe.br/bibdigital/2013/10.12.16.06 3
sid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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