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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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