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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/JwF7G
Repositorysid.inpe.br/iris@1916/2005/12.21.12.50   (restricted access)
Last Update2005:12.22.12.12.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/12.21.12.50.10
Metadata Last Update2018:06.05.01.16.38 (UTC) administrator
Secondary KeyINPE-13070-PRE/8334
ISSN0378-4371
Citation KeyAndradeWuenRibe:2005:CoMiAd
TitleCorrelated mixture between adiabatic and isocurvature fluctuations and recent CMB observations
Year2005
MonthFEB
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size3098 KiB
2. Context
Author1 Andrade, Ana Paula de Almeida
2 Wuensche, Carlos Alexandre
3 Ribeiro, André Luís Batista
Group1 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE, DAS)
JournalPhysica A: Statistical Mechanics and its Applications
Volume71
Number4
PagesArt. No. 043501
History (UTC)2005-12-22 12:13:03 :: vinicius -> administrator ::
2008-06-10 22:41:13 :: administrator -> banon ::
2010-05-17 18:17:10 :: banon -> administrator ::
2018-06-05 01:16:38 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsPROBE WMAP OBSERVATIONS
COSMOLOGICAL PARAMETERS
INFLATIONARY UNIVERSE
POWER SPECTRUM
GAUSSIANITY
AbstractThis work presents a reduced chi(nu)(2) test to search for non-Gaussian signals in the cosmic microwave background radiation (CMBR) TT power spectrum of recent CMBR data, Wilkinson Anisotropy Microwave Probe, Arcminute Cosmology Bolometer Array Receiver, and Cosmic Background Imager data sets, assuming a mixed density field including adiabatic and isocurvature fluctuations. We assume a skew positive mixed model with adiabatic inflation perturbations plus additional isocurvature perturbations possibly produced by topological defects. The joint probability distribution used in this context is a weighted combination of Gaussian and non-Gaussian random fields. Results from simulations of CMBR temperature for the mixed field show a distinct signature in CMB power spectrum for very small deviations (similar to0.1%) from a pure Gaussian field, and can be used as a direct test for the nature of primordial fluctuations. A reduced chi(nu)(2) test applied on the most recent CMBR observations reveals that an isocurvature fluctuations field is not ruled out and indeed permits a very good description for a flat geometry Lambda-CDM Universe, chi(930)(2)similar to1.5, rather than the simple inflationary standard model with chi(930)(2)similar to2.3. This result may looks is particular discrepant with the reduced chi(2) of 1.07 obtained with the same model in Spergel et al. [Astrophys. J. 148, 175 (2003)] for temperature only, however, our work is restricted to a region of the parameter space that does not include the best fit model for TT only of Spergel et al.. .
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Correlated mixture between...
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4. Conditions of access and use
Languageen
Target FileCorrelated mixture between.pdf
User Groupadministrator
banon
vinicius
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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