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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3MPQ2PS
Repositorysid.inpe.br/mtc-m21b/2016/11.11.15.40   (restricted access)
Last Update2016:11.11.15.40.20 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2016/11.11.15.40.20
Metadata Last Update2018:06.04.02.41.15 (UTC) administrator
DOI10.1140/epjc/s10052-016-4327-y
ISSN1434-6044
Citation KeyAraújoCoelCost:2016:GrWaPu
TitleGravitational waves from pulsars with measured braking index
Year2016
MonthAug.
Access Date2024, May 12
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size985 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 DAS-CEA-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
JournalEuropean Physical Journal C
Volume76
Number9
Secondary MarkA2_INTERDISCIPLINAR A2_BIOTECNOLOGIA A2_ASTRONOMIA_/_FÍSICA B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_ENGENHARIAS_IV
History (UTC)2016-11-11 15:40:40 :: simone -> administrator :: 2016
2016-11-14 05:25:47 :: administrator -> simone :: 2016
2016-12-21 12:04:00 :: simone -> administrator :: 2016
2018-06-04 02:41:15 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe study the putative emission of gravitational waves (GWs) in particular for pulsars with measured braking index. We show that the appropriate combination of both GW emission and magnetic dipole brakes can naturally explain the measured braking index, when the surface magnetic field and the angle between the magnetic dipole and rotation axes are time dependent. Then we discuss the detectability of these very pulsars by aLIGO and the Einstein Telescope. We call attention to the realistic possibility that aLIGO can detect the GWs generated by at least some of these pulsars, such as Vela, for example.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Gravitational waves from...
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
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Visibilityshown
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
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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