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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/485EBAS
Repositorysid.inpe.br/mtc-m21d/2022/12.02.18.49
Last Update2022:12.02.18.49.39 (UTC) simone
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Metadata Last Update2023:01.03.16.46.26 (UTC) administrator
DOI10.1093/mnras/stac2159
ISSN0035-8711
1365-2966
Citation KeyDantas:2022:MeEnRa
TitleMesoscopic energy ranking constraints in the IllustrisTNG simulations
Year2022
Access Date2024, May 13
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5820 KiB
2. Context
AuthorDantas, Christine Córdula
GroupDIAST-CGCE-INPE-MCTI-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addressccordulad@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume516
Pages279-297
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2022-12-02 18:49:40 :: simone -> administrator ::
2022-12-02 18:49:40 :: administrator -> simone :: 2022
2022-12-02 18:49:47 :: simone -> administrator :: 2022
2023-01-03 16:46:26 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitation –methods: numerical –galaxies: formation –galaxies: haloes –galaxies: kinematics and dynamics –cosmology: dark matter
AbstractWe revisited the problem of mixing in a gravitational N -body system from the point of view of the ordering of coarse-grained cells in the one-particle energy space, here denoted energy ranking preservation (ERP). This effect has been noted for some time in simulations, although individual particle energies and their phase-space variables mix considerably. The present investigation aimed to map ERP in terms of parameters involving the collective range in which it is effective, as well as in terms of global and historical characterizations of gravitational systems evolving towards equilibrium. We examined a subset of the IllustrisTNG cosmological magnetohydrodynamical simulations (TNG50-4 and TNG100-3), considering both their full and dark-only v ersions. F or each simulation, we selected the 20 most massiv e haloes at redshift z = 0, tracing their ERP fractions back at selected redshift markers ( z = { 1.0, 5.0, 10 0 } ), and for a coarse-graining set ranging from 5 to 30 energy bins. At the redshift marker z = 1, we found high ERP fractions (abo v e ∼80 per cent ) in both simulations, regardless of the coarse-graining level. The decline in ERP fractions with redshift was roughly a function of mass and fractional mass increase in the analysed TNG50-4 haloes, but not in the TNG100-3 ones, indicating a possible relative susceptibility of the ERP effect to mass accretion for haloes less massive than ∼10 14 M . We confirmed earlier indications in the literature concerning a possible mesoscopic constraint operative in a time span of at least several Gyr.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Mesoscopic energy ranking...
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data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/485EBAS
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/485EBAS
Languageen
Target File2022_ASTRO_DANTAS_Kandrup_MNRAS_stac2159.pdf
User Groupsimone
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Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
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