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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/485STN2
Repositorysid.inpe.br/mtc-m21d/2022/12.05.15.45   (restricted access)
Last Update2022:12.05.15.45.21 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/12.05.15.45.21
Metadata Last Update2023:01.03.16.46.26 (UTC) administrator
DOI10.1088/1742-6596/2372/1/012002
ISSN1742-6588
Citation KeyNovaesBeneBern:2022:PrNoIn
TitlePrimordial non-gaussianities of inflationary step-like models
Year2022
Access Date2024, May 13
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size3567 KiB
2. Context
Author1 Novaes, Camila Paiva
2 Benetti, M.
3 Bernui, A.
Group1 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Università di Napoli “Federico II”
3 Observatório Nacional (ON)
Author e-Mail Address1 camilapnovaes@gmail.com
JournalJournal of Physics: Conference Series
Volume2372
Number1
Pagese012002
Secondary MarkB2_INTERDISCIPLINAR B2_ENGENHARIAS_III B3_MEDICINA_II B3_GEOCIÊNCIAS B4_MATERIAIS B4_ENGENHARIAS_II B4_BIOTECNOLOGIA C_QUÍMICA C_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA C_ENGENHARIAS_IV C_ECONOMIA C_ASTRONOMIA_/_FÍSICA
History (UTC)2022-12-05 15:45:21 :: simone -> administrator ::
2022-12-05 15:45:22 :: administrator -> simone :: 2022
2022-12-05 15:46:09 :: 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
AbstractWe use Minkowski Functionals (MF) to explore the possible presence of non-Gaussian signatures in the recently released cosmic microwave background (CMB) Planck maps. In particular, we investigate MF outcomes for two sets of simulated CMB maps: one seeded by the ΛCDM concordance model, another seeded by the 'best-fit' CMB angular power spectrum. By 'best-fit' we mean a simulated CMB spectrum seeded by an inflationary model that well reproduce the observed low-ℓ features of the CMB temperature power spectrum. In this way, we obtain the spurious signal introduced by the power spectra with different shapes, signal to be taken into account in the corresponding MF analyses. Interestingly, we investigate the response of the four MF (i.e., Area, Perimeter, Genus, Nclusters ) for several sets of simulated maps. Our analyses confirm that, as already reported in the literature, the Perimeter exhibits the best performance. Moreover, our results show that the Perimeter obtained from the Planck maps (2015) is better fitted by the simulated CMB maps seeded by the angular power spectrum with low-ℓ features with respect to the curves obtained from the CMB maps seeded by the ΛCDM model.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Primordial non-gaussianities of...
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4. Conditions of access and use
Languageen
Target FileNovaes_2022_J._Phys.__Conf._Ser._2372_012002.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
Notes18th Meeting of Physics, MOPHY 2019Lima, 15-16 Aug. 2019
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository month nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
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