1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZQjxQKY/GpvEB |
Repository | sid.inpe.br/ePrint@80/2005/06.09.12.25 (restricted access) |
Last Update | 2005:08.30.17.12.14 (UTC) administrator |
Metadata Repository | sid.inpe.br/ePrint@80/2005/06.09.12.25.42 |
Metadata Last Update | 2018:06.04.04.12.43 (UTC) administrator |
Secondary Key | INPE-12548-PRE/7846 |
DOI | 10.1016/j.astropartphys.2004.12.004 |
ISSN | 1475-7516 |
Citation Key | Araujo:2005:DaEnUn |
Title | The dark energy-dominated Universe |
Project | Ondas gravitacionais / Gráviton |
Year | 2005 |
Secondary Date | 2004 |
Month | Mar. |
Access Date | 2024, May 11 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 312 KiB |
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2. Context | |
Author | Araujo, Jose Carlos Neves de |
Resume Identifier | 8JMKD3MGP5W/3C9JHGK |
Group | DAS-INPE-MCT-BR |
Affiliation | Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) |
Author e-Mail Address | jcarlos@das.inpe.br |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 23 |
Number | 2 |
Pages | 279-286 |
History (UTC) | 2010-05-14 01:58:01 :: alexandra -> administrator :: 2018-06-04 04:12:43 :: administrator -> marciana :: 2005 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Keywords | ASTROPHYSICS Cosmology theory Cosmological parameters Cosmological constant Dark energy Dark matter Cosmological constant Lambda ASTROFÍSICA Teoria cosmológica Parâmetros cosmológicos Constante cosmológica Energia escura Matéria escura |
Abstract | In 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The dark energy-dominated... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Target File | dark energy.pdf |
User Group | administrator alexandra |
Visibility | shown |
Copy Holder | SID/SCD |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Dissemination | WEBSCI; PORTALCAPES. |
Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
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6. Notes | |
Empty Fields | alternatejournal 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 |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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