The Role of Fragmentation (cont)
Performed simulations with 1m ≤ rf ≤ 100m with resolution of 0.5 dex. For our gas disk we find:
- For rf ≥ 30m, resonant trapping pushed planet inward
little growth.
- For rf ≤ 3m, fragments swept by planets little growth.
- Only for rf = 10m do we find a significant amount of growth:
- However, fragments likely follow ~ a power law SFD, so we expect little mass in sweet-spot.
