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Cosmological Dark Halos History From the formalism of Reed et al
(MNRAS, 346, 565-572, 2003) it is calculated the mass fraction of dark
matter halos. The code obtain the mass density of dark halos and the
fraction of brions into structures as a function of the time. Here is
used the Transfer function from Efstathiou, Bond & White -- (MNRAS,
258, 1P, 1992). The current version it is assumed the normalization of
WMAP (withou gravitational waves) adapted from Eisenstein e Hu (ApJ 511,
5, 1999) that in the way that return sigma_8 = 0,84. The fraction of
mass of dark halos is obtained by the work of Sheth e Tormen (MNRAS 308,
119, 1999). All models consider Omega_Total = Omega_M + Omega_L = 1,0
This file is part of pystar. copyright : Eduardo dos Santos
Pereira
pystar is free software: you can redistribute it and/or modify it
under the terms of the GNU General Public License as published by the
Free Software Foundation, either version 3 of the License. pystar is
distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY;
without even the implied warranty of MERCHANTABILITY or FITNESS FOR A
PARTICULAR PURPOSE. See the GNU General Public License for more
details.
You should have received a copy of the GNU General Public License
along with Foobar. If not, see <http://www.gnu.org/licenses/>.
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