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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/475K5N8
Repositorysid.inpe.br/mtc-m21d/2022/06.20.19.13
Last Update2022:06.20.19.13.39 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/06.20.19.13.39
Metadata Last Update2023:01.03.16.46.08 (UTC) administrator
DOI10.1093/mnras/stac1445
ISSN0035-8711
1365-2966
Citation KeyAllahyariNuneMota:2022:SlGrLi
TitleNo slip gravity in light of LISA standard sirens
Year2022
MonthJune
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1158 KiB
2. Context
Author1 Allahyari, Alireza
2 Nunes, Rafael da Costa
3 Mota, David F.
Group1
2 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Institute for Research in Fundamental Sciences (IPM)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 University of Oslo
Author e-Mail Address1 alireza.al@ipm.ir
2 rafadcnunes@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume514
Number1
Pages1274-1281
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2022-06-20 19:13:39 :: simone -> administrator ::
2022-06-20 19:13:40 :: administrator -> simone :: 2022
2022-06-20 19:14:05 :: simone -> administrator :: 2022
2023-01-03 16:46:08 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitation
gravitational waves
cosmology: observations
dark energy
AbstractStandard sirens (SS) are the gravitational wave analogue of the astronomical standard candles, and can provide powerful information about the dynamics of the Universe up to very high z values. In this work, we generate three mock SS catalogues based on the merger of massive black hole binaries which are expected to be observed in the LISA operating frequency band. Then, we perform an analysis to test modifications of general relativity (GR) inspired by the no slip gravity framework. We find that in the best scenarios, we can constrain the free parameters which quantify deviations from GR to 21 per cent accuracy, while the Hubble parameter can be simultaneously fit to 6 per cent accuracy. In combination with CMB information, we find a 15 per cent accuracy on the modified gravity free parameters and 0.7 per cent accuracy on the Hubble parameter. The SS events at very large cosmological distances to be observed in LISA band will provide a unique way to test nature of gravity, but in the context of the analysis performed here, it will not be possible to distinguish the no slip gravity from GR.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > No slip gravity...
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source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/475K5N8
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/475K5N8
Languageen
Target Filestac1445.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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