Table 2.
Nonideal amplification of the different component (gas-gas, star-star, and gas-star) for two different values of the threshold gth used to define the bound radius.
| Case 1 | ||||
|---|---|---|---|---|
| gth | 1 | 4 | ||
| αgg | 5.02 | 15.56 | ||
| αgs | 6.28 | 21.0 | ||
| αss | 61.0 | 257 | ||
| Xstar | 0.05 | 0.1 | 0.05 | 0.1 |
| αni | 5.28 | 5.80 | 16.7 | 18.9 |
| Hni | 34.2 | 35.8 | 60.7 | 64.7 |
 |
0.12 | 0.13 | 0.20 | 0.21 |
| qni | −1.20 | −1.21 | −1.12 | −1.09 |
| Case 2 | ||||
| gth | 1 | 4 | ||
| αgg | 16.4 | 36.2 | ||
| αgs | 31.7 | 72.7 | ||
| αss | 61.0 | 257 | ||
| Xstar | 0.05 | 0.1 | 0.05 | 0.1 |
| αni | 17.9 | 19.6 | 40.2 | 45.0 |
| Hni | 62.9 | 65.8 | 94.3 | 94.3 |
 |
0.21 | 0.21 | 0.26 | 0.27 |
| qni | −1.09 | −1.09 | −0.87 | −0.83 |
Notes. Total nonideal amplification αni and the corresponding nonideal Hubble parameter (Hni in units of km s−1 Mpc−1) for two different values of the star mass fraction relative to the total baryon mass in the Universe (we assume a present-day baryon density of 0.25 particle/m3). Estimation of 
assuming a 14 Gyr old Universe and the corresponding nonideal deceleration parameter qni.
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