@Article{PereiraMira:2015:RoDaMa,
author = "Pereira, Eduardo dos Santos and Miranda, Oswaldo Duarte",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "The role of the dark matter haloes on the cosmic star formation
rate",
journal = "New Astronomy",
year = "2015",
volume = "41",
pages = "48--52",
month = "Nov.",
keywords = "(Cosmology):dark matter, Stars: formation, Stars: general,
Galaxies: star formation.",
abstract = "The cosmic star formation rate (CSFR) represents the fraction of
gas that is converted into stars within a certain comoving volume
and at a given time t. However the evolution of the dark matter
haloes and its relationship with the CSFR is not yet clear. In
this context, we have investigated the role of the dark halo mass
function - DHMF - in the process of gas conversion into stars. We
observed a strong dependence between the fraction of baryons in
structures, fb, and the specific mass function used for describing
the dark matter haloes. In some cases, we have obtained fb greater
than one at redshift z=0. This result indicates that the evolution
of dark matter, described by the specific DHMF, could not trace
the baryonic matter without a bias parameter. We also observed
that the characteristic time-scale for star formation, \τ,
is strongly dependent on the considered DHMF, when the model is
confronted against the observational data. Also, as part of this
work it was released, under GNU general public license, a Python
package called pycosmicstar to study the CSFR and its relationship
with the DHMF.",
doi = "10.1016/j.newast.2015.06.001",
url = "http://dx.doi.org/10.1016/j.newast.2015.06.001",
issn = "1384-1076",
language = "en",
targetfile = "pereira_the role.pdf",
urlaccessdate = "27 abr. 2024"
}