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1. Identity statement
Reference TypeBook Section
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4AJJ7Q5
Repositorysid.inpe.br/mtc-m21d/2024/01.19.18.41   (restricted access)
Last Update2024:01.19.18.41.55 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2024/01.19.18.41.55
Metadata Last Update2024:01.27.06.27.33 (UTC) administrator
Secondary KeyINPE--/
DOI10.1142/9789811269776_0377
ISBN9789811269776
Citation KeySousaAraúCoel:2023:GrWaFa
TitleGravitational waves from fast-spinning white dwarfs
Year2023
Access Date2024, June 15
Secondary TypePRE LI
Number of Files1
Size762 KiB
2. Context
Author1 Sousa, Manoel Felipe
2 Araújo, José Carlos Neves de
3 Coelho, Jaziel G.
Resume Identifier1
2 8JMKD3MGP5W/3C9JHGK
Group1 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
2 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Tecnológica Federal do Paraná (UTFPR)
Author e-Mail Address1 manoel.sousa@inpe.br
2 jcarlos.dearaujo@inpe.br
3 jazielcoelho@utfpr.edu.br
EditorRuffini, R.
Vereshchagin, G.
Book TitleThe Sixteenth Marcel Grossmann Meeting. On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories
PublisherWorld Scientific Publishing
Pages4461-4474
History (UTC)2024-01-19 18:42:21 :: simone -> administrator :: 2023
2024-01-27 06:27:33 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGravitational Waves
White Dwarfs
Magnetic Field
Rapid Rotation
AbstractWe discuss some aspects of Sousa et al. [1, 2] concerning two mechanisms of gravitational wave (GW) emission in fast-spinning white dwarfs (WDs): accretion of matter and magnetic deformation. In both cases, the GW emission is generated by an asymmetry around the rotation axis of the star. However, in the first case, the asymmetry is due to the amount of accreted matter in the magnetic poles, while in the second case it is due to the intense magnetic field. We have estimated the GW amplitude and luminosity for three binary systems that have a fast-spinning magnetized WD, namely, AE Aquarii, AR Scorpii and RX J0648.0-4418. In addition, we applied the magnetic deformation mechanism for SGRs/AXPs described as WD pulsars. We found that, for the first mechanism, the systems AE Aquarii and RX J0648.0-4418 can be observed by the space detectors BBO and DECIGO if they have an amount of accreted mass of δm ≥ 10−5M⊙. For the second mechanism, the three systems studied require that the WD has a magnetic field above ∼ 109 G to emit GWs that can be detected by BBO. Furthermore, we found that some SGRs/AXPs as WD pulsars can be detected by BBO and DECIGO, whereas SGRs/AXPs as highly magnetized neutron stars are far below the sensitivity curves of these detectors.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Gravitational waves from...
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4. Conditions of access and use
Languageen
Target Filesousa-et-al-2023-gravitational-waves-from-fast-spinning-white-dwarfs.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
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5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 3
sid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
DisseminationBNDEPOSITOLEGAL
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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