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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/U9sjM
Repositorysid.inpe.br/mtc-m17@80/2008/05.14.11.04   (restricted access)
Last Update2008:05.14.11.04.51 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2008/05.14.11.04.52
Metadata Last Update2018:06.05.03.30.41 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1103/PhysRevD.77.083516
ISSN0378-4371
Citation KeyCostaAlcaMaia:2008:CoQuVa
TitleCoupled quintessence and vacuum decay
Year2008
MonthApril
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size192 KiB
2. Context
Author1 Costa, F. E. M.
2 Alcaniz, J. S.
3 Maia, J. M. F.
Group1
2 CRN-CIE-INPE-MCT-BR
Affiliation1 Observatório Nacional. Departamento de Astronomia
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 CNPq. COAIE
JournalPhysica A: Statistical Mechanics and its Applications
Volume77
History (UTC)2008-07-18 12:09:27 :: rosemary -> banon ::
2008-11-04 18:43:15 :: banon -> administrator ::
2010-05-11 02:43:30 :: administrator -> banon ::
2010-05-17 19:10:30 :: banon -> administrator ::
2018-06-05 03:30:41 :: administrator -> rosemary :: 2008
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsCoupled quintessence
Vacuum decay
COSMOLOGY
AbstractWe discuss observational consequences of a class of cosmological models characterized by the dilution of pressureless matter attenuated with respect to the usual a-3 scaling due to the decay of vacuum energy. We carry out a joint statistical analysis of observational data from the new gold sample of 182 SNe Ia, recent estimates of the cosmic microwave background shift parameter, and baryon acoustic oscillations measurements from the SDSS to show that such models favor the decay of vacuum only into the dark matter sector, and that the separately conserved baryons cannot be neglected. In order to explore ways to more fundamentally motivate these models, we also derive a coupled scalar field version for this general class of vacuum decay scenarios..
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRN > Coupled quintessence and...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileCoupled quintessence.pdf
User Groupadministrator
banon
rosemary
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EUAPES
DisseminationWEBSCI; PORTALCAPES.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
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