Table 2
Statistical results of population synthesis calculations.
| Name | “Hot” | “Cold” | Total massive | “Hot” massive | “Cold” massive | |
|
|
||||||
| BMF model, reference synthesis | 54.4 | 45.6 | 13.3 | 4.0 | 9.3 | |
| isothermal migration model | 79.2 | 20.8 | 7.8 | 2.7 | 5.1 | |
| BMF model, Casoli Lind. | 48.8 | 51.2 | 15.0 | 2.9 | 12.1 | |
| RED model | 35.4 | 64.6 | 19.1 | 1.4 | 17.7 | |
| STD model | 60.5 | 39.5 | 11.4 | 4.5 | 6.9 | |
| Paardekooper, free gamma | 55.4 | 44.6 | 12.0 | 4.1 | 7.9 | |
| Paardekooper, gamma = 1.4 | 59.3 | 40.7 | 9.5 | 4.1 | 5.4 | |
| BMF model, irradiated disks | 68.8 | 31.2 | 10.1 | 3.8 | 6.3 | |
Notes. In the first seven syntheses simulation we consider 6850 planets more massive than 0.6 M⊕. In the synthesis with the irradiated disk we consider ≈7700 planets more massive than 0.6 M⊕. The second column shows the percentage of planets that migrated to 0.1 AU (“hot” planets), while the third column corresponds to “cold” planets (a> 0.1 AU).We also show the fraction of embryos that grow more massive than 100 M⊕ (total massive) and how they split into “hot” and “cold” massive planets in columns four to six.
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