Table 1
Model parameters and outcome of the simulations.
| Label | Bound(a) | Res(b) | M1 (c) | M2 (c) | facc | Σ (d) | Migration(e) | Jump(f) | Events(g) | Fig. | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| M9-3, A0.0 | O | 9 | 3 | ↗ | ✓ | (h) | |||||
| M6-2 | O | 6 | 2 | ↗ | ✓ | ||||||
| M3-1 | O | 3 | 1 | ↗ | ✓ | ||||||
| M9-4.5 | O | 9 | 4.5 | ↗ | ✓ | DS | 3 | ||||
| M6-3 | O | 6 | 3 | ↗ | ✓ | ||||||
| M6-6 | O | 6 | 6 | ↘ | 3 | ||||||
| M3-9 | O | 3 | 9 | ↘ | 3 | ||||||
| M2-6 | O | 2 | 6 | ↘ | |||||||
| M3-1.5 | O | 3 | 1.5 | ↘ | |||||||
| M9-3 HR | O | 1/2 | 9 | 3 | ↗ | ✓ | A.1 | ||||
| M9-3 DR | O | 2 | 9 | 3 | ↗ | ✓ | A.1 | ||||
| M9-3 M/10 | O | 9 | 3 | 1/10 | ↗ | ||||||
| IRR | O | 9 | 3 | ↗ | ✓ | B.1, B.2 | |||||
| FLARE | O | 9 | 3 | ↗ | ✓ | B.1, B.2 | |||||
| A0.0001 | O | 9 | 3 | 10−4 | ↗ | ✓ | 7, 8 | ||||
| A0.001 | O | 9 | 3 | 10−3 | ↗ | ✓ | 7, 8 | ||||
| A0.01 | O | 9 | 3 | 10−2 | ↗ | ✓ | DS | 7, 8 | |||
| A0.1 | O | 9 | 3 | 10−1 | ↗ | ✓ | 7, 8 | ||||
| L | O | 1/2 | 9 | 3 | ↗ ↘ | ✓ | S | 9 | |||
| L M/2 | O | 1/2 | 9 | 3 | 1/2 | ↗ | ✓ | ||||
| L M/10 | O | 1/2 | 9 | 3 | 1/10 | ↗ | |||||
| VB | V | 9 | 3 | ↗ | ✓ | E | |||||
| VB5 | V5 | 9 | 3 | ↗ | ✓ | E | |||||
| WD | O+WD | 1/2 | 9 | 3 | ↗ | ✓ | E | ||||
| WDR | R+WD | 1/2 | 9 | 3 | ↗ | ✓ | E | ||||
| VB-P | V | 9 | 3 | ↗ | ✓ | ||||||
| VB5-P | V5 | 9 | 3 | ↗ | ✓ | ||||||
| WD-P | O+WD | 1/2 | 9 | 3 | ↗ | ✓ | |||||
| WDR-P | R+WD | 1/2 | 9 | 3 | ↗ | ✓ | |||||
| SG | V5 | 9 | 3 | ↗ ↘ | ✓ | S | |||||
| SG IRR | V5 | 9 | 3 | ↗ ↘ | ✓ | DS, S | |||||
| PDS70 ISO | O | 9 | 3 | ↗ | ✓ | 11 | |||||
| PDS70 IRR | O | 9 | 3 | ↗ | ✓ | 11 | |||||
| PDS70 IRR M/5 | O | 9 | 3 | 1/5 | ↗ | 11 | |||||
Notes. If a field is empty in the Res, facc, or Σ column, the values are the same as for the reference model M9-3. (a)For the inner boundary, the following choices are possible: O means an outflow boundary, R a closed reflective boundary, V a viscous boundary, V5 a viscous boundary with five times viscous speed, and +WD indicates an additional wave damping zone close to the inner boundary, see Sect. 2.4 for more detail. (b) The factor refers to the 2D resolution compared to the M9-3 case (Sect. 2.2). (c) Planet masses in units of MJup. (d) Surface density in units of the reference density Σ0 (see Eq. (1)). (e)Direction of migration where ↗ and ↘ indicate outward and inward migration, respectively. (f) ✓, if at least one migration jump happened in the simulation. (g) Additional events of interest, where S indicates a single orbit swap, DS a double orbit swap, and E stands for planet ejection. (h) The standard model M9-3 is used in Figs. 3, 4, 5, 6, 8, A.1, B.1, B.2, 6 and C.1.
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