Open Access

Table A.2.

Fiducial parameters used in simulations.

Stellar (Solar-type)
Mass M 1.0 M
Radius R 1.0 R (0.00465 au)
Disrupted Jupiter-like planet
Total mass Mp 0.99 MJup
Layers (atmosphere / mantle / core) Mi 0.65 / 0.32 / 0.02 MJup
Disruption radii (Roche) r0, i = RRoche, i 0.012 / 0.009 / 0.0056 au

VEPs (volatile-enriched planets)
Mass Mp 1, 10 M
Semi-major axis a 0.04, 0.07 au
Hill radius RH = a (Mp/3M)1/3 4.0 × 10−4 au (1 M)
1.5 × 10−4 au (10 M)
Capture radius Rcap = 0.2 RH 8.0 × 10−5 au (1 M)
3.0 × 10−5 au (10 M)

Disc and hydrodynamic simulation
Kinematic viscosity ν 7 × 1013 cm2 s−1
Radial domain [rin, rout] [0.001, 0.10] au
Resolution (Nr, Nϕ) (720, 1024)
Equation of state locally isothermal

Kelvin–Helmholtz contraction
Rosseland mean opacity κR 1 cm2 g−1
Exponent 1 − 1/q −2.5
Exponent s/q 1
Time-scale tKH ∼ 108 (Mcore/M)−2.5 yr

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