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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44QAMML
Repositorysid.inpe.br/mtc-m21c/2021/06.02.12.39
Last Update2021:06.02.12.39.45 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2021/06.02.12.39.45
Metadata Last Update2022:04.03.19.24.45 (UTC) administrator
DOI10.1093/mnras/stab445
ISSN0035-8711
1365-2966
Citation KeyDantas:2021:RoBaPh
TitleCounts-in-cells of subhaloes in the IllustrisTNG simulations: The role of baryonic physics
Year2021
MonthApr.
Access Date2025, June 02
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1157 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
Volume502
Number4
Pages5495-5507
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)2021-06-02 12:39:45 :: simone -> administrator ::
2021-06-02 12:39:46 :: administrator -> simone :: 2021
2021-06-02 12:39:54 :: simone -> administrator :: 2021
2022-04-03 19:24:45 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsdark matter
galaxies: clusters: general
large-scale structure of Universe
AbstractWe present an analysis of the counts-in-cells (CiC) statistics of subhaloes in the publicly available IllustrisTNG cosmological simulations (TNG100-1, TNG100-3, and TNG300-3), considering their full and dark-only versions, in redshifts ranging from z = 0 to z = 5, and different cell sizes. We evaluated two CiC models: the gravitational quasi-equilibrium distribution (GQED) and the negative binomial distribution (NBD), both presenting good fits, with small detectable differences in the presence of baryons. Scaling and time dependencies of the best-fitting parameters showed similar trends compared with the literature. We derived a matter density-in-cells probability distribution function (PDF), associated with the GQED, which was compared to the PDF proposed by Uhlemann et al., for the IllustrisTNG 100-3-Dark run at z = 0. Our results indicate that the simplest gravithermodynamical assumptions of the GQED model hold in the presence of baryonic dissipation. Interestingly, the smoothed (density-in-cells) version of the GQED is also adequate for describing the dark matter one-point statistics of subhaloes and converges, to subpercentage levels (for an interval of parameters), to the Uhlemann et al. PDF in the high density range.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Counts-in-cells of subhaloes...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/44QAMML
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/44QAMML
Languageen
Target Filedantas_counts.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 6
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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