Table 1.

The bifrost user-given parameters relevant for simulations of this study. The parameter definitions correspond to the ones in Rantala et al. (2023).

bifrost user-given parameterSymbolValue
Forward integrator time-step factor|$\eta _\mathrm{{ff}},\eta _\mathrm{{fb}},\eta _\mathrm{{\nabla }}$|0.2
Subsystem neighbour radius|$r_\mathrm{{rgb}}$|10 |$\mathrm{mpc}$|
Regularization GBS tolerance|$\eta _\mathrm{{GBS}}$||$10^{-7}$|
Regularization GBS end-time tolerance|$\eta _\mathrm{{endtime}}$|0.01
Regularization highest PN order PN3.5
Secular integration threshold|$N_{\mathrm{orb,sec}}$|0
Secular highest PN order PN2.5
bifrost user-given parameterSymbolValue
Forward integrator time-step factor|$\eta _\mathrm{{ff}},\eta _\mathrm{{fb}},\eta _\mathrm{{\nabla }}$|0.2
Subsystem neighbour radius|$r_\mathrm{{rgb}}$|10 |$\mathrm{mpc}$|
Regularization GBS tolerance|$\eta _\mathrm{{GBS}}$||$10^{-7}$|
Regularization GBS end-time tolerance|$\eta _\mathrm{{endtime}}$|0.01
Regularization highest PN order PN3.5
Secular integration threshold|$N_{\mathrm{orb,sec}}$|0
Secular highest PN order PN2.5
Table 1.

The bifrost user-given parameters relevant for simulations of this study. The parameter definitions correspond to the ones in Rantala et al. (2023).

bifrost user-given parameterSymbolValue
Forward integrator time-step factor|$\eta _\mathrm{{ff}},\eta _\mathrm{{fb}},\eta _\mathrm{{\nabla }}$|0.2
Subsystem neighbour radius|$r_\mathrm{{rgb}}$|10 |$\mathrm{mpc}$|
Regularization GBS tolerance|$\eta _\mathrm{{GBS}}$||$10^{-7}$|
Regularization GBS end-time tolerance|$\eta _\mathrm{{endtime}}$|0.01
Regularization highest PN order PN3.5
Secular integration threshold|$N_{\mathrm{orb,sec}}$|0
Secular highest PN order PN2.5
bifrost user-given parameterSymbolValue
Forward integrator time-step factor|$\eta _\mathrm{{ff}},\eta _\mathrm{{fb}},\eta _\mathrm{{\nabla }}$|0.2
Subsystem neighbour radius|$r_\mathrm{{rgb}}$|10 |$\mathrm{mpc}$|
Regularization GBS tolerance|$\eta _\mathrm{{GBS}}$||$10^{-7}$|
Regularization GBS end-time tolerance|$\eta _\mathrm{{endtime}}$|0.01
Regularization highest PN order PN3.5
Secular integration threshold|$N_{\mathrm{orb,sec}}$|0
Secular highest PN order PN2.5
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