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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PTQQBE
Repositorysid.inpe.br/mtc-m21b/2017/11.03.14.08   (restricted access)
Last Update2017:11.03.14.08.50 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/11.03.14.08.50
Metadata Last Update2018:06.04.02.27.57 (UTC) administrator
DOI10.1142/S2010194517600060
ISSN2010-1945
Citation KeyGontijoMira:2017:ExMaWa
TitleExcitation magnetohydrodynamic wave by gravitational wave produced by binary of neutron stars
Year2017
Access Date2024, June 16
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size338 KiB
2. Context
Author1 Gontijo, Adam Smit
2 Miranda, Oswaldo Duarte
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
Group1 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 adam.assis@inpe.br
2 oswaldo.miranda@inpe.br
JournalInternational Journal of Modern Physics: Conference Series
Volume45
Secondary MarkB4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2017-11-03 14:12:59 :: simone -> administrator :: 2017
2018-06-04 02:27:57 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsMagnetohydrodynamics Wave
Gravitational Wave
Gamma-Ray Bursts
AbstractThe gravitational wave, through the strongly magnetized plasma surrounding the neutron stars, in the z-direction, deforms plasma particle rings in ellipses, alternating axes periodically along the direction of the magnetic field (x-axis) and of the y-axis. The uniform field leads to a modulation of the magnetic field, which results in magnetic pressure gradients (magneto-acoustic mode) or in the shear of the magnetic field lines (Alfv´en mode). The gravitational wave drives MHD modes and transfers energy to the plasma, can become an important alternative process for the acceleration of baryons to high Lorentz factors observed in short GRBs. The total amount of energy that is transferred from the gravitational wave to the plasma is estimated (' 1040J - 1041 J), with γ ' 102 . We compare our results with previously obtained results by other works.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Excitation magnetohydrodynamic wave...
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4. Conditions of access and use
Languageen
Target Filegontijo_excitation.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher allowfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.32 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
Notes7th International Workshop on Astronomy and
Relativistic Astrophysics (IWARA 2016)
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository month nextedition number orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
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