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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/39RQCKS
Repositorydpi.inpe.br/plutao/2011/06.11.03.13   (restricted access)
Last Update2011:12.06.17.00.30 (UTC) tereza@sid.inpe.br
Metadata Repositorydpi.inpe.br/plutao/2011/06.11.03.13.22
Metadata Last Update2018:06.05.00.01.18 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.physletb.2011.05.022
ISSN0370-2693
Labellattes: 6217296674061205 3 AlvesMiraArau:2011:CaMaGr
Citation KeyAlvesMiraArau:2011:CaMaGr
TitleCan massive gravitons be an alternative to dark energy?
ProjectFAPESP 06/03158-0/CNPq 300713/2009-6 e 305823/2010-8
Year2011
MonthJunho
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size251 KiB
2. Context
Author1 Alves, M. E. S.
2 Miranda, Oswaldo Duarte
3 de Araujo, Jose Carlos Neves
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
3 8JMKD3MGP5W/3C9JHGK
Group1
2 DAS-CEA-INPE-MCT-BR
3 DAS-CEA-INPE-MCT-BR
Affiliation1 Universidade Federal Itajuba
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 alvesmes@unifei.edu.br
2 oswaldo@das.inpe.br
3 jcarlos@das.inpe.br
e-Mail Addressjcarlos@das.inpe.br
JournalPhysics Letters B
Volume700
Number5
Pages283-288
History (UTC)2011-06-11 17:43:44 :: lattes -> marciana :: 2011
2011-11-01 11:21:21 :: marciana -> tereza@sid.inpe.br :: 2011
2011-12-06 17:00:39 :: tereza@sid.inpe.br -> administrator :: 2011
2012-07-25 15:50:24 :: administrator -> banon :: 2011
2012-09-27 18:02:26 :: banon -> administrator :: 2011
2012-10-19 20:25:34 :: administrator -> tereza@sid.inpe.br :: 2011
2013-03-04 18:24:57 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 00:01:18 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGRAVITATIONAL-WAVES
COSMOLOGY
MODEL
AbstractIn this work, we explore some cosmological implications of the model proposed by M. Visser in 1998. In his approach. Visser intends to take into account mass for the graviton by means of an additional bimetric tensor in the Einstein's field equations. Our study has shown that a consistent cosmological model arises from the Visser's approach. The most interesting feature is that an accelerated expansion phase naturally emerges from the cosmological model, and we do not need to postulate any kind of dark energy to explain the current observational data for distant type la supernovae (SNIa). (C) 2011 Elsevier B.V. All rights reserved.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Can massive gravitons...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
User Groupadministrator
banon
lattes
marciana
tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
URL (untrusted data)http://www.sciencedirect.com/science/article/pii/S0370269311005284
DisseminationPORTALCAPES
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
NotesSetores de Atividade: Pesquisa e desenvolvimento científico.
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork
7. Description control
e-Mail (login)tereza@sid.inpe.br
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