Table 5
Parameters different from the standard parameters in Table 3 that are used for simulations in Sect. 4.
| Parameter | Values |
|---|---|
| ϵ0 | 0.01, 0.015, 0.02, 0.025 |
| α | 1 × 10−4, 5 × 10−4, 1 × 10−3 |
| tevap | 1 Myr, 2 Myr, 3 Myr |
| t0 | 0.05 Myr, 0.15 Myr, 0.25 Myr, 0.35 Myr, 0.45 Myr |
| ap,0 | 1 AU, 2 AU, 3 AU, 5 AU, 10 AU, 15 AU, 20 AU, 25 AU, 30 AU |
Notes. Simulations are performed on a grid by simulating each of the 1620 possible combinations. Like Thorngren et al. (2016), only planets with final masses in the range of 20 M⊕ and 20 MJ and stellar insulations less than F⋆ < 2 × 108 erg s−1 cm−2 and additionally only planets with final orbits with less than 1 AU are considered (except in Fig. 15).
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