Table 1: Summary of the main parameters of the cosmological numerical simulations.
Cosmology $\Omega_{\rm m}$a $\Omega_{\Lambda}$b $\Omega_{\rm b}$c ${\rm H_0}$d $\sigma_{8}$e $N_{\rm g}$f $N_{\rm d}$g Lh
$\Lambda $CDM 0.30 0.70 0.04 70 0.90 803 803 10
SCDM 1.00 0.00 0.10 50 0.62 26214 235930 5
a $\Omega_{\rm m}$: mass density parameter.
b $\Omega_{\Lambda}$: vacuum energy density parameter.
c $\Omega_{\rm b}$: baryonic density parameter.
d H0: Hubble constant.
e $\sigma_{8}$: rms density fluctuations at 8 Mpc h-1.
f $N_{\rm g}$: initial number of gas particles.
g $N_{\rm d}$: total number of dark matter particles.
h L: box size of the simulated volume Mpc h-1.

Source LaTeX | All tables | In the text