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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3B58JHL
Repositorysid.inpe.br/mtc-m19/2012/01.02.16.06   (restricted access)
Last Update2012:01.03.18.00.36 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/01.02.16.06.26
Metadata Last Update2018:06.05.04.25.13 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1142/S0218271811020433
ISSN0218-2718
Citation KeyFillouxPachDuriArau:2011:DeRaLI
TitleCoalescence Rate of Supermassive Black Hole Binaries derived from cosmolgical simulations: Detection rates for LISA and ET
Year2011
MonthNov
Access Date2024, May 04
Secondary TypePRE PI
Number of Files1
Size441 KiB
2. Context
Author1 Filloux, C. H.
2 Pacheco, J. A. de Freitas
3 Durier, F.
4 Araujo, José Carlos Neves de
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHGK
Group1
2
3
4 DAS-CEA-INPE-MCT-BR
Affiliation1 Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Cassiopee
2 Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Cassiopee
3 Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
4 Instituto Nacional de Pesquisas Espaciais (INPE)
e-Mail Addresssecretaria.cpa@dir.inpe.br
JournalInternational Journal of Modern Physics D
Volume20
Number12
Pages2399-2417
Secondary MarkB2_ASTRONOMIA_/_FÍSICA B1_ENGENHARIAS_III A2_INTERDISCIPLINAR B2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2012-01-02 16:06:26 :: secretaria.cpa@dir.inpe.br -> administrator ::
2012-01-02 16:06:27 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2012-01-03 18:01:54 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2018-06-05 04:25:13 :: administrator -> marciana :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGravitational waves
supermassive black holes
cosmological simulations
AbstractThe coalescence history of massive black holes has been derived from cosmological simulations, in which the evolution of those objects and that of the host galaxies are followed in a consistent way. The present study indicates that supermassive black holes having masses greater than similar to 10(9) M(circle dot) underwent up to 500 merger events along their history. The derived coalescence rate per comoving volume and per mass interval permitted to obtain an estimate of the expected detection rate distribution of gravitational wave signals ("ring-down") along frequencies accessible by the planned interferometers either in space (LISA) or in the ground (Einstein). For LISA, in its original configuration, a total detection rate of about 15 yr(-1) is predicted for events having a signal-to-noise ratio equal to 10, expected to occur mainly in the frequency range 4-9mHz. For the Einstein gravitational wave telescope, one event each 14 months down to one event each four years is expected with a signal-to-noise ratio of 5, occurring mainly in the frequency interval 10-20Hz. The detection of these gravitational signals and their distribution in frequency would be in the future an important tool able to discriminate among different scenarios explaining the origin of supermassive black holes.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Coalescence Rate of...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
User Groupadministrator
secretaria.cpa@dir.inpe.br
Visibilityshown
Archiving Policydenypublisher allowfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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