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Table 1
Key simulation parameters.
| Symbol | Value | Quantity |
|---|---|---|
| M* | 1 M⊙ | Stellar mass |
| R* | 2.08 R⊙ | Stellar radius |
| T* | 4000 K | Stellar surface temperature |
| α | 0.001 | Shakura-Sunyaev |
| viscosity parameter | ||
| µ | 2.3 | Mean molecular weight of gas |
| γ | 1.41 | Adiabatic index of gas |
| cd | 0.7 Jg−1K−1 | Specific heat capacity of dust |
| c𝑔 | 8.8 Jg−1K−1 | Specific heat capacity of gas |
| {nr, nθ, nϕ} | 134,58,460 | Cells along each dimension (low-resolution, 1000 orbits) |
 |
268,116,919 | Cells along each dimension (high-resolution, 10 orbits) |
| {rin, rout} | {16 au, 100 au} | Inner and outer radial boundaries |
| {θlow, θup} | {−0.4,0.4} + π/2 | Lower and upper polar boundaries |
| rinf | 18 au | Outer boundary of inner wave-damping zone |
| rsup | 95 au | Inner boundary of outer wave-damping zone |
| rp | 40 au | Planet radius |
 |
40 y | Dynamical time at rp |
| 3 × 10−4 M⊙ | Mass of Saturn | |
| 1 × 10−3 M⊙ | Mass of Jupiter |
Notes. More information can be found in Sect. 2.1.3 of this work and in Sect. 2 of Muley et al. (2024).
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