%0 Book Section
%2 sid.inpe.br/mtc-m21c/2020/02.10.17.23.38
%4 sid.inpe.br/mtc-m21c/2020/02.10.17.23
%3 pereira_towards.pdf
%A Pereira, Eduardo dos Santos,
%A Santos, Pedro Alexandre dos,
%A Campos Velho, Haroldo Fraga de,
%@secondarytype PRE LI
%B Integral methods in science and engineering
%C Brighton, UK
%D 2019
%E Constanda, Christian,
%E Harris, Paul,
%@secondarykey INPE--PRE/
%I Springer
%K black holes.
%P 333-342
%T Towards the super-massive black hole seeds
%X In 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.
%@area COMP
%@electronicmailaddress eduardo.santos@inpe.br
%@electronicmailaddress pedro.alexandre@inpe.br
%@electronicmailaddress haroldo.camposvelho@inpe.br
%@documentstage not transferred
%@group COCST-COCST-INPE-MCTIC-GOV-BR
%@group LABAC-COCTE-INPE-MCTIC-GOV-BR
%@group LABAC-COCTE-INPE-MCTIC-GOV-BR
%@isbn 978-3-030-16077-7
%@usergroup simone
%@resumeid
%@resumeid
%@resumeid 8JMKD3MGP5W/3C9JHC3
%@nexthigherunit 8JMKD3MGPCW/3ESGTTP
%@nexthigherunit 8JMKD3MGPCW/3F3T29H
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@versiontype publisher
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}