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Table 1
Parameters and settings for the model.
Quantity | Value |
|
|
Stellar mass | 1 M⊙ |
Disk viscosity parameter α | 7 × 10-3 |
Disk photoevaporation | int. & external (Paper II) |
Irradiation for disk temperature profile | included |
Number of embryos per disk | 1 |
Embryo starting mass | 0.6 M⊕ |
Core accretion rate | Alibert et al. (2005) |
Planetesimal size | 100 km |
Fate of dissolved planetesimals | sink to core interface |
Core density | variable (Paper II) |
Envelope type | primordial H2/He |
Envelope evaporation | not included |
Atmosphere type during evolution | Eddington gray (Paper I) |
ISM grain opacity reduction factor | 0.003 |
Radiogenic luminosity | included |
Deuterium burning | included |
Accretion shock luminosity treatment | fully cold/hot accretion |
∂l/∂r in the envelope | zero |
Simulation duration | 10 Gyr |
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