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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/LwSqM
Repositorysid.inpe.br/mtc-m16@80/2006/06.22.13.17   (restricted access)
Last Update2006:06.22.13.17.48 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/06.22.13.17.49
Metadata Last Update2018:06.05.01.16.51 (UTC) administrator
Secondary KeyINPE-13803--PRE/8989
ISSN0923-2958
Citation KeyDantasRamo:2006:GrMeCo
TitleGravitational mesoscopic constraints in cosmological dark matter halos
Year2006
MonthJan.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size158 KiB
2. Context
Author1 Dantas, Christine C.
2 Ramos, Fernando Manuel
Resume Identifier1
2 8JMKD3MGP5W/3C9JH4A
Group1 LAC-INPE-MCT-BR
Affiliation1 Instituto de Aeronáutica e Espaço (IAE/CTA)
2 Instituto Nacional de Pesquisas Espaciais, Laboratório Associado de Computação e Matermática Aplicada
JournalCelestial Mechanics and Dynamical Astronomy
Volume94
Number1
Pages67-81
History (UTC)2006-06-22 13:17:49 :: simone -> administrator ::
2008-06-10 22:42:44 :: administrator -> simone ::
2011-05-21 13:13:46 :: simone -> administrator ::
2018-06-05 01:16:51 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsdark matter halos
fundamental plane of elliptical galaxies
N-body simulations
scaling relations
DISSIPATIONLESS GALAXY FORMATION
FUNDAMENTAL PLANE
ELLIPTIC GALAXIES
STATISTICAL-MECHANICS
VIOLENT RELAXATION
STELLAR-SYSTEMS
MERGERS
SIMULATIONS
LAW
AbstractWe present an analysis of the behaviour of the ` coarse- grained' (`mesoscopic') rank partitioning of the mean energy of collections of particles composing virialized dark matter halos in a Lambda-CDM cosmological simulation. We find evidence that rank preservation depends on halo mass, in the sense that more massive halos show more rank preservation than less massive ones. We find that the most massive halos obey Arnold's theorem ( on the ordering of the characteristic frequencies of the system) more frequently than less massive halos. This method may be useful to evaluate the coarse- graining level ( minimum number of particles per energy cell) necessary to reasonably measure signatures of ` mesoscopic' rank orderings in a gravitational system.
AreaCOMP
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAC > Gravitational mesoscopic constraints...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target FileGravitational mososcopic constraints in cosmological.pdf
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simone
Visibilityshown
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Update Permissiontransferred to simone
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ESGTTP
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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