1. Identity statement | |
Reference Type | Journal Article |
Site | plutao.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | J8LNKAN8RW/39RQCKS |
Repository | dpi.inpe.br/plutao/2011/06.11.03.13 (restricted access) |
Last Update | 2011:12.06.17.00.30 (UTC) tereza@sid.inpe.br |
Metadata Repository | dpi.inpe.br/plutao/2011/06.11.03.13.22 |
Metadata Last Update | 2018:06.05.00.01.18 (UTC) administrator |
Secondary Key | INPE--PRE/ |
DOI | 10.1016/j.physletb.2011.05.022 |
ISSN | 0370-2693 |
Label | lattes: 6217296674061205 3 AlvesMiraArau:2011:CaMaGr |
Citation Key | AlvesMiraArau:2011:CaMaGr |
Title | Can massive gravitons be an alternative to dark energy? |
Project | FAPESP 06/03158-0/CNPq 300713/2009-6 e 305823/2010-8 |
Year | 2011 |
Month | Junho |
Access Date | 2024, May 02 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 251 KiB |
|
2. Context | |
Author | 1 Alves, M. E. S. 2 Miranda, Oswaldo Duarte 3 de Araujo, Jose Carlos Neves |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JJ2G 3 8JMKD3MGP5W/3C9JHGK |
Group | 1 2 DAS-CEA-INPE-MCT-BR 3 DAS-CEA-INPE-MCT-BR |
Affiliation | 1 Universidade Federal Itajuba 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 alvesmes@unifei.edu.br 2 oswaldo@das.inpe.br 3 jcarlos@das.inpe.br |
e-Mail Address | jcarlos@das.inpe.br |
Journal | Physics Letters B |
Volume | 700 |
Number | 5 |
Pages | 283-288 |
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 Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | GRAVITATIONAL-WAVES COSMOLOGY MODEL |
Abstract | In 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Can massive gravitons... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
|
4. Conditions of access and use | |
Language | en |
User Group | administrator banon lattes marciana tereza@sid.inpe.br |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
|
5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
URL (untrusted data) | http://www.sciencedirect.com/science/article/pii/S0370269311005284 |
Dissemination | PORTALCAPES |
Host Collection | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
|
6. Notes | |
Notes | Setores de Atividade: Pesquisa e desenvolvimento científico. |
Empty Fields | alternatejournal 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 |
update | |
|