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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3ARN9HG
Repositorydpi.inpe.br/plutao/2011/11.23.17.27.50   (restricted access)
Last Update2011:12.23.18.36.53 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/11.23.17.27.51
Metadata Last Update2021:07.28.22.06.41 (UTC) administrator
DOI10.1111/j.1745-3933.2011.01137.x
ISSN1745-3933
Labellattes: 9527086189389353 2 PereiraMira:2011:CoGrCo
Citation KeyPereiraMira:2011:CoGrCo
TitleSupermassive black holes: connecting the growth to the cosmic star formation rate
ProjectCNPq 300713/2009-6
Year2011
MonthNov 2011
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size9 KiB
2. Context
Author1 Pereira, Eduardo dos Santos
2 Miranda, Oswaldo Duarte
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
Group1 DAS-CEA-INPE-MCT-BR
2 DAS-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 duducosmo@das.inpe.br
2 oswaldo@das.inpe.br
e-Mail Addressoswaldo@das.inpe.br
JournalMonthly Notices of the Royal Astronomical Society Letters
Volume418
Number1
PagesL30-L34
History (UTC)2011-11-24 11:03:15 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2012-01-17 15:58:42 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2021-07-28 22:06:41 :: administrator -> marciana :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsblack hole physics
galaxies: active
galaxies: evolution
galaxies: nuclei
quasars: general
AbstractWe present a model connecting the cosmic star formation rate (CSFR) to the growth of supermassive black holes. Considering that the evolution of the massive black hole is dominated by accretion (Soltans argument) and that the accretion process can be described by a probabilistic function directly regulated by the CSFR, we obtain the evolution of the black hole mass density. Then, using the quasar luminosity function, we determine both the functional form of the radiative efficiency and the evolution of the quasar duty cycle as functions of the redshift. We analyse four different CSFRs showing that the quasar duty cycle, d(z), peaks at z similar to 8.511 and so within the window associated with the reionization of the Universe. In particular, dmax similar to 0.090.22 depending on the CSFR. The mean radiative efficiency, , peaks at z similar to 0.11.3 with depending on the specific CSFR used. Our results also show that it is not necessary for a supercritical Eddington accretion regime to produce the growth of the black hole seeds. The present scenario is consistent with the formation of black hole seeds similar to 103 M? at z similar to 20.
AreaCEA
Arrangementurlib.net > Fonds > Produção anterior à 2021 > DIDAS > Supermassive black holes:...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
User Groupadministrator
lattes
secretaria.cpa@dir.inpe.br
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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