Table 4: Concentration and perturbation asymptotic growth factor in the different cosmologies.
cosmology $\displaystyle\frac{c_0} {c_0^{\rm\Lambda CDM}}$ $\displaystyle\frac{D_+(\infty)} {D_+^{\rm\Lambda CDM}(\infty)}$ $\displaystyle\frac{D_+(z_{\rm coll})} {D_+^{\rm\Lambda CDM}(z_{\rm coll})}$

${\rm\Lambda CDM}$ 1 1 1

RP $1.06\pm0.011$ 1.07 $1.07\pm0.0003$

SUGRA $1.16\pm0.013$ 1.22 $1.19\pm0.004$

DECDM $1.18\pm0.013$ 1.19 $1.18\pm0.001$

OCDM $1.49\pm0.018$ 1.64 $1.61\pm0.01$

**Table 4:** Concentration and perturbation asymptotic growth factor in the different cosmologies.
cosmology	$\displaystyle\frac{c_0} {c_0^{\rm\Lambda CDM}}$	$\displaystyle\frac{D_+(\infty)} {D_+^{\rm\Lambda CDM}(\infty)}$	$\displaystyle\frac{D_+(z_{\rm coll})} {D_+^{\rm\Lambda CDM}(z_{\rm coll})}$
${\rm\Lambda CDM}$	1	1	1
RP	$1.06\pm0.011$	1.07	$1.07\pm0.0003$
SUGRA	$1.16\pm0.013$	1.22	$1.19\pm0.004$
DECDM	$1.18\pm0.013$	1.19	$1.18\pm0.001$
OCDM	$1.49\pm0.018$	1.64	$1.61\pm0.01$

Source LaTeX | All tables | In the text