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Table 5
Input parameters used to run the modified GroMiT code to produce the synthetic planetary populations shown in Fig. 14. Half of the simulations adopt a pebble size of 1 cm, and the other half adopt a size of 1 mm.
| Simulation parameters | |
|---|---|
| N° of simulations | 6×104 |
| Seed formation time | 0.1–1 × 106 yr |
| Disk lifetime | 5 × 106 yr |
| Star, planet & disk properties | |
| Stellar Mass | 0.756 M⊙ |
| Seed Mass | 0.01 M⊕ |
| Initial envelope mass | 0.0 M⊕ |
| Initial semimajor axis | 0.1–30.0 au |
| Disk characteristic radius | 30.0 au |
| Temperature at 1 au | 150K |
| Surface density at 30 au | 490 kg m−2 |
| Disk accretion coefficient, α | 0.01 |
| Turbulent viscosity, αν | 0.0001 |
| Pebble size | 1 cm & 1 mm |
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