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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3T7F5H2
Repositorysid.inpe.br/mtc-m21c/2019/04.26.15.54
Last Update2019:04.26.15.54.09 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/04.26.15.54.09
Metadata Last Update2020:01.06.11.42.13 (UTC) administrator
DOI10.1103/PhysRevD.99.084022
ISSN1550-2368
1550-7998
Citation KeyNunesAlveAraú:2019:PrGrWa
TitlePrimordial gravitational waves in Horndeski gravity
Year2019
MonthApr.
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size603 KiB
2. Context
Author1 Nunes, Rafael da Costa
2 Alves, Márcio E. S.
3 Araújo, José Carlos Neves de
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHGK
Group1 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
2
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Estadual Paulista (UNESP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 rafadcnunes@gmail.com
2 marcio.alves@unesp.br
3 jcarlos.dearaujo@inpe.br
JournalPhysical Review D
Volume99
Number8
Pages084022
Secondary MarkA2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B2_ENSINO B2_ENGENHARIAS_IV B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2019-04-26 15:54:09 :: simone -> administrator ::
2019-04-26 15:54:10 :: administrator -> simone :: 2019
2019-04-26 15:54:37 :: simone -> administrator :: 2019
2020-01-06 11:42:13 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe investigate the propagation of primordial gravitational waves within the context of the Homdeski theories; for this, we present a generalized transfer function quantifying the subhorizon evolution of gravitational wave modes after they enter the horizon. We compare the theoretical prediction of the modified primordial gravitational wave spectral density with the aLIGO, Einstein telescope, LISA, gLISA and DECIGO sensitivity curves. Assuming reasonable and different values for the free parameters of the theory (in agreement with the event GW170817 and stability conditions of the theory), we note that the gravitational wave amplitude can vary significantly in comparison with general relativity. We find that in some cases the gravitational primordial spectrum can cross the sensitivity curves for the DECIGO detector with the maximum frequency sensitivity to the theoretical predictions around 0.05-0.30 Hz. From our results, it is clear that the future generations of space based interferometers can bring new perspectives to probing modifications in general relativity.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Primordial gravitational waves...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Primordial gravitational waves...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3T7F5H2
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3T7F5H2
Languageen
Target Filenunes_primordial.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3F2NE4L
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 4
sid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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