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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3TKAMTB
Repositorysid.inpe.br/mtc-m21c/2019/07.08.11.21
Last Update2019:08.05.12.19.57 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/07.08.11.21.19
Metadata Last Update2020:01.06.11.42.16 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyNunesAlveAraú:2019:PrGrWa
TitlePrimordial gravitational waves in horndeski gravity
Year2019
Access Date2024, May 13
Secondary TypePRE CI
Number of Files1
Size603 KiB
2. Context
Author1 Nunes, R. C.
2 Alves, M. E. S.
3 Araújo, José Carlos Neves de
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHGK
Group1
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
2
3 jcarlos.dearaujo@inpe.br
Conference NameInternational Conference on General Relativity and Gravitation
Conference LocationValencia, Spain
Date07-12 july
History (UTC)2019-07-08 11:21:59 :: simone -> administrator :: 2019
2019-07-10 01:45:52 :: administrator -> simone :: 2019
2019-08-05 12:19:58 :: simone -> administrator :: 2019
2020-01-06 11:42:16 :: 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 Horndeski theories, for this, we present a generalized transfer function quantifying the sub-horizon evolution of gravitational waves modes after they enter the horizon. We compare the theoretical prediction of the modified primordial gravitational waves 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 waves 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 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
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Primordial gravitational waves...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3TKAMTB
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3TKAMTB
Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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7. Description control
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