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Fig. 12

image

Outcome of single-planet formation simulations with the default setting (i.e. (b, c) = (8, 3) for the Kelvin–Helmholtz timescale, [Fe/H] = 0.0, and the pebble accretion efficiency by IGM16) with αturb = 10−3 (left panels),10−4 (middle panels), and 10−5 (right panels). The top panels show the final semi-major axis of a single planet for different initial semi-major axes and disc models. The bottom cells marked as ‘Init’ correspond to the initial semi-major axes that are common for all disc models. The bottom panels present the final planetary masses in log scale. The bottom cells represent the initial protoplanetary masses of 0.01M for all the cases.

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