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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/42FHABB
Repositorysid.inpe.br/mtc-m21c/2020/05.12.12.24   (restricted access)
Last Update2020:05.12.12.24.12 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/05.12.12.24.12
Metadata Last Update2022:01.04.01.35.08 (UTC) administrator
DOI10.1088/1475-7516/2020/03/015
ISSN1475-7516
Citation KeyBonillaDAgoNuneAraú:2020:FoSpGr
TitleForecasts on the speed of gravitational waves at high z
Year2020
MonthMar.
Access Date2024, May 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2986 KiB
2. Context
Author1 Bonilla, Alexander
2 D'Agostino, Rocco
3 Nunes, Rafael da Costa
4 Araújo, José Carlos Neves de
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHGK
Group1
2
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
4 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Federal de Juiz de Fora (UFJF)
2 Università di Napoli
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 abonilla@fisica.ufjf.br
2 rdagostino@na.infn.it
3 rafadcnunes@gmail.com
4 jcarlos.dearaujo@inpe.br
JournalJournal of Cosmology and Astroparticle Physics
Volume3
Pagese015
Secondary MarkA1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA B1_GEOCIÊNCIAS
History (UTC)2020-05-12 12:24:12 :: simone -> administrator ::
2020-05-12 12:24:13 :: administrator -> simone :: 2020
2020-05-12 12:24:55 :: simone -> administrator :: 2020
2022-01-04 01:35:08 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitational waves / sources
modified gravity
AbstractThe observation of GW170817 binary neutron star (BNS) merger event has imposed strong bounds on the speed of gravitational waves (GWs) locally, inferring that the speed of GWs propagation is equal to the speed of light. Current GW detectors in operation will not be able to observe BNS merger to long cosmological distance, where possible cosmological corrections on the cosmic expansion history are expected to play an important role, specially for investigating possible deviations from general relativity. Future GW detectors designer projects will be able to detect many coalescences of BNS at high z, such as the third generation of the ground GW detector called Einstein Telescope (ET) and the space-based detector deci-hertz interferometer gravitational wave observatory (DECIGO). In this paper, we relax the condition c(T)/c = 1 to investigate modified GW propagation where the speed of GWs propagation is not necessarily equal to the speed of light. Also, we consider the possibility for the running of the Planck mass corrections on modified GW propagation. We parametrize both corrections in terms of an effective GW luminosity distance and we perform a forecast analysis using standard siren events from BNS mergers, within the sensitivity predicted for the ET and DECIGO. We find at high z very strong forecast bounds on the running of the Planck mass, namely O (10(-1)) and O(10(-2)) from ET and DECIGO, respectively. Possible anomalies on GW propagation are bound to vertical bar c(T)/c - 1 vertical bar <= 10(-2) (10(-2)) from ET (DECIGO), respectively. We finally discuss the consequences of our results on modified gravity phenomenology.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Forecasts on the...
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Languageen
Target Filebonilla_forecasts.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
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Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
DisseminationWEBSCI; PORTALCAPES.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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