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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZQjxQKY/GpvEB
Repositorysid.inpe.br/ePrint@80/2005/06.09.12.25   (restricted access)
Last Update2005:08.30.17.12.14 (UTC) administrator
Metadata Repositorysid.inpe.br/ePrint@80/2005/06.09.12.25.42
Metadata Last Update2018:06.04.04.12.43 (UTC) administrator
Secondary KeyINPE-12548-PRE/7846
DOI10.1016/j.astropartphys.2004.12.004
ISSN1475-7516
Citation KeyAraujo:2005:DaEnUn
TitleThe dark energy-dominated Universe
ProjectOndas gravitacionais / Gráviton
Year2005
Secondary Date2004
MonthMar.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size312 KiB
2. Context
AuthorAraujo, Jose Carlos Neves de
Resume Identifier8JMKD3MGP5W/3C9JHGK
GroupDAS-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
Author e-Mail Addressjcarlos@das.inpe.br
JournalJournal of Cosmology and Astroparticle Physics
Volume23
Number2
Pages279-286
History (UTC)2010-05-14 01:58:01 :: alexandra -> administrator ::
2018-06-04 04:12:43 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsASTROPHYSICS
Cosmology theory
Cosmological parameters
Cosmological constant
Dark energy
Dark matter
Cosmological constant
Lambda
ASTROFÍSICA
Teoria cosmológica
Parâmetros cosmológicos
Constante cosmológica
Energia escura
Matéria escura
AbstractIn this paper we investigate the epochs in which the Universe started accelerating and when it began to become dark energy-dominated (i.e., the dynamics of the expansion of the Universe dominated by the dark energy). We provide analytic expressions to calculate the redshifts of these epochs as a function of density parameters. Moreover, we review and discuss cosmological models with a dark energy component, which can have an interesting characteristic, namely, they never stop accelerating. This holds even if the Universe is at present time either flat, open, or closed. If the dark energy is the cosmological constant the Universe will eventually end up undergoing an exponentially expansion phase, and the total density parameter converging to Omega = 1. This is exactly what is considered in inflationary scenario to generate the initial conditions for the big bang. One can then argue that the Universe begun with an inflationary phase and will end up with another inflationary phase. Thus, it follows that in both the early and the late Universe Omega -> 1. We also discuss the above issues in the context of the XCDM parametrization.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The dark energy-dominated...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Target Filedark energy.pdf
User Groupadministrator
alexandra
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage e-mailaddress format isbn label language lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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