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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3U9E2FH
Repositorysid.inpe.br/mtc-m21c/2019/10.21.18.52
Last Update2019:10.21.18.52.47 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/10.21.18.52.47
Metadata Last Update2020:01.06.11.42.23 (UTC) administrator
DOI10.1103/PhysRevD.100.064012
ISSN1550-2368
1550-7998
Citation KeyNunesAlveAraú:2019:FoCoT
TitleForecast constraints on f (T) gravity with gravitational waves from compact binary coalescences
Year2019
MonthSept.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size934 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 DIDAS-CGCEA-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
Volume100
Number6
Pagese64012
Secondary MarkA2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B2_ENSINO B2_ENGENHARIAS_IV B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2019-10-21 18:52:47 :: simone -> administrator ::
2019-10-21 18:52:53 :: administrator -> simone :: 2019
2019-10-21 18:53:29 :: simone -> administrator :: 2019
2020-01-06 11:42:23 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe direct detection of gravitational waves (GWs) opened a new chapter in the modern cosmology to probe possible deviations from the general relativity (GR) theory. In the present work, we investigate for the first time the modified GW form propagation from the inspiraling of compact binary systems within the context of fðTÞ gravity in order to obtain new forecasts/constraints on the free parameter of the theory. First, we show that the modified waveform differs from the GR waveform essentially due to induced corrections on the GWs amplitude. Then, we discuss the forecasts on the fðTÞ gravity assuming simulated sources of GWs as black hole binaries, neutron star binaries and black holeneutron star binary systems, which emit GWs in the frequency band of the Advanced LIGO (aLIGO) interferometer and of the third generation Einstein Telescope (ET). We show that GW sources detected within the aLIGO sensitivity can return estimates of the same order of magnitude of the current cosmological observations. On the other hand, detection within the ET sensitivity can improve by up to 2 orders of magnitude the current bound on the fðTÞ gravity. Therefore, the statistical accuracy that can be achieved by future ground based GW observations, mainly with the ET detector (and planed detectors with a similar sensitivity), can allow strong bounds on the free parameter of the theory, and can be decisive to test the theory of gravitation.
AreaCEA
ArrangementForecast constraints on...
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/3U9E2FH
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3U9E2FH
Languageen
Target Filenunes_forecast.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
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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