Table A.1
Present-epoch parameters characterising marginally collapsing objects in comparison to those at turn-around for various cosmological models. See text for an explanation of the listed parameters.
| Label | Ωm | h | R | H ov | Δc | R | Δc |
| future collapse | at turn-around | ||||||
|
|
|||||||
| – | 0.24 | 0.7 | 9.811 | 17.60 | 1.36 | 14.31 | 2.43 |
| – | 0.27 | 0.7 | 8.732 | 19.09 | 1.36 | 13.12 | 2.54 |
| – | 0.30 | 0.7 | 7.858 | 20.55 | 1.36 | 12.15 | 2.65 |
| – | 0.33 | 0.7 | 7.134 | 22.00 | 1.35 | 11.35 | 2.75 |
| WMAPa | 0.288 | 0.697 | 8.188 | 19.89 | 1.36 | 12.52 | 2.60 |
| Planck b | 0.318 | 0.670 | 7.409 | 20.50 | 1.36 | 11.66 | 2.71 |
| – | 0.27 | 0.60 | 8.732 | 16.36 | 1.36 | 13.12 | 2.54 |
| EdS | 1.0 | 0.7 | – | – | – | 5.54 | 4.54 |
| open | 0.3 | 0.7 | 2.87 | 52.70 | 12.48 | ||
Notes.
Best fit for the combined model in Hinshaw et al. (2013);
best fit for Planck and WMAP polarisation data (Planck Collaboration XVI, 2014).
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