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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36HLAEL
Repositorysid.inpe.br/mtc-m19@80/2009/12.09.18.30   (restricted access)
Last Update2009:12.09.18.30.29 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.09.18.30.31
Metadata Last Update2018:06.05.04.36.00 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1088/1475-7516/2009/09/031
ISSN1475-7516
Citation KeyBessadaKinnTzir:2009:InPoDB
TitleInflationary potentials in DBI models
Year2009
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size445 KiB
2. Context
Author1 Bessada, Dennis
2 Kinney, William H.
3 Tzirakis, Konstantinos
Group1 DAS-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 University at Buffalo
3 University at Buffalo
JournalJournal of Cosmology and Astroparticle Physics
Volume31
History (UTC)2010-03-15 11:48:58 :: simone -> administrator ::
2018-06-05 04:36:00 :: administrator -> marciana :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsinflation
alternatives to inflation
AbstractWe study DBI inflation based upon a general model characterized by a power-law flow parameter () á and speed of sound cs() â, where á and â are constants. We show that in the slow-roll limit this general model gives rise to distinct inflationary classes according to the relation between á and â and to the time evolution of the inflaton field, each one corresponding to a specific potential; in particular, we find that the well-known canonical polynomial (large- and small-field), hybrid and exponential potentials also arise in this non-canonical model. We find that these non-canonical classes have the same physical features as their canonical analogs, except for the fact that the inflaton field evolves with varying speed of sound; also, we show that a broad class of canonical and D-brane inflation models are particular cases of this general non-canonical model. Next, we compare the predictions of large-field polynomial models with the current observational data, showing that models with low speed of sound have red-tilted scalar spectrum with low tensor-to-scalar ratio, in good agreement with the observed values. These models also show a correlation between large non-gaussianity with low tensor amplitudes, which is a distinct signature of DBI inflation with large-field polynomial potentials.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Inflationary potentials in...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileinflationary.pdf
User Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark month 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
e-Mail (login)marciana
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