Close

1. Identity statement
Reference TypeBook Section
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UTKC8P
Repositorysid.inpe.br/mtc-m21c/2020/02.10.17.23   (restricted access)
Last Update2020:02.10.17.23.38 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/02.10.17.23.38
Metadata Last Update2022:03.15.18.56.38 (UTC) administrator
Secondary KeyINPE--PRE/
ISBN978-3-030-16077-7
Citation KeyPereiraSantCamp:2019:ToSuBl
TitleTowards the super-massive black hole seeds
Year2019
Access Date2024, May 05
Secondary TypePRE LI
Number of Files1
Size345 KiB
2. Context
Author1 Pereira, Eduardo dos Santos
2 Santos, Pedro Alexandre dos
3 Campos Velho, Haroldo Fraga de
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHC3
Group1 COCST-COCST-INPE-MCTIC-GOV-BR
2 LABAC-COCTE-INPE-MCTIC-GOV-BR
3 LABAC-COCTE-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 eduardo.santos@inpe.br
2 pedro.alexandre@inpe.br
3 haroldo.camposvelho@inpe.br
EditorConstanda, Christian
Harris, Paul
Book TitleIntegral methods in science and engineering
PublisherSpringer
CityBrighton, UK
Pages333-342
History (UTC)2020-02-10 17:23:38 :: simone -> administrator ::
2022-03-15 18:56:38 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsblack holes
AbstractIn science, there are different problems to be solved. One of them is the evolution of the Universe. This paper discusses a little piece of the cited problem, which is the evolution of the black holes. From nowadays, observations show super-massive black holes with mass about 109M3 are ubiquitous in galaxy centers. However, the origin of this kind of object is not completely understood yet. A possibility rely in the fact the super-massive black holes (SMBH) seeds had their origin in the death of the Population III stars, during the called Dark Cosmological Ages at redshift in the interval z = [10, 20]. In order to verify this hypothesis, the first step is to try to reconstruct the SMBH mass function at high redshift. The next step is to do a comparison between the computed distribution with the reminiscent of the first stars.
AreaCOMP
ArrangementTowards the super-massive...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 10/02/2020 14:23 1.8 KiB 
4. Conditions of access and use
Languageen
Target Filepereira_towards.pdf
User Groupsimone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3F3T29H
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition format issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor seriestitle session shorttitle sponsor subject tertiarymark tertiarytype translator url volume
7. Description control
e-Mail (login)simone
update 


Close