Fig. 9

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Comparison of our model to results from the code comparison project in FNS19. Evolution of an initially 2 planet inserted at 120 au. Left: mass vs. time; right: separation vs. time. The green shaded region represents the region of parameter space covered by six different hydrodynamic codes. The results from our calculation are shown as thick dotted and dash-dotted lines (legend in the right panel). Results from different disc instability population synthesis codes are also shown (legend in the left panel). The grey shaded-hatched region corresponds to the region of parameter space covered by Nayakshin & Fletcher (2015). The orange dashed line shows the result from Forgan & Rice (2013). The result from Müller et al. (2018) is shown in blue. The dotted line (covered by the solid line in the left panel) represents a different gap opening criterion (see details in Sect. 4.8).
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