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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/48BJ225
Repositorysid.inpe.br/mtc-m21d/2023/01.09.12.32
Last Update2023:01.09.12.33.31 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/01.09.12.32.29
Metadata Last Update2023:01.10.17.38.30 (UTC) administrator
DOI10.1103/PhysRevD.106.124053
ISSN1550-2368
1550-7998
Citation KeyDAgostinoNune:2022:FoCoDe
TitleForecasting constraints on deviations from general relativity in f (Q) gravity with standard sirens
Year2022
MonthDec
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size632 KiB
2. Context
Author1 D'Agostino, Rocco
2 Nunes, Rafael da Costa
ORCID1 0000-0003-2342-1134
2 0000-0002-8432-5616
Group1
2 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Scuola Superiore Meridionale (SSM)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 rafadcnunes@gmail.com
JournalPhysical Review D
Volume106
Number12
Pagese124053
Secondary MarkA2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B2_ENSINO B2_ENGENHARIAS_IV B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2023-01-09 12:32:29 :: simone -> administrator ::
2023-01-09 12:32:30 :: administrator -> simone :: 2022
2023-01-09 12:33:32 :: simone -> administrator :: 2022
2023-01-10 17:38:30 :: administrator -> simone :: 2022
3. Content and structure
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Content TypeExternal Contribution
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AbstractIn this work, we explore how modified gravity theories based on the nonmetricity scalar, known as f(Q) gravity, affect the propagation of gravitational waves from inspiraling of binary systems. We discuss forecast constraints on f(Q) gravity by considering standard siren events in two contexts: (i) simulated sources of gravitational waves as black hole-neutron star binary systems, emitting in the frequency band of the third-generation detector represented by the Einstein Telescope (ET); (ii) three standard siren mock catalogs based on the merger of massive black hole binaries that are expected to be observed in the operating frequency band of the Laser Interferometer Space Antenna (LISA). We find that, within the ET sensitivity, in combination with supernova and cosmic chronometer data, it will be possible to test deviations from general relativity at <3% accuracy in the redshift range 0<z<5, while the main free parameter of the theory is globally constrained at 1.6% accuracy within the same range. In light of LISA's forecasts, combined to supernova and cosmic chronometer data, in the best scenario, we find that the main free parameter of the theory will be constrained at 1.6% accuracy up to high redshifts. Therefore, we conclude that future gravitational wave observations by ET and LISA will provide a unique way to test, with good accuracy, the nature of gravity up to very large cosmic distances.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Forecasting constraints on...
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/48BJ225
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/48BJ225
Languageen
Target FilePhysRevD.106.124053.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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