H-He mass fraction after 3 Myr (upper panels), 5 Myr (middle panels), and 10 Myr (lower panels). The left panels show in situ formation at 3 au and the right panels at 5 au. The colors indicate the heavy-element interaction models. Case-1, Case-2, Case-3, and Case-4 are given in red, blue, purple, and yellow, respectively. The three different solid accretion rates are distinguished by different symbols. We also show the light initial disk results by a transparent marker, the medium disk result with a 0.5 opacity marker, and the heavy disk result with a full opacity marker. The light, medium and heavy results of the same model are connected by a line, as we would expect that in intermediate disk would produce a final H-He fraction approximately along this line. The total masses in the figure are limited to below 15 M_⊕, focusing on the distribution for mini-Neptune type planets. Planets that reached the crossover mass (M_env = M_core) are not shown, even if their total mass is below 15 M_⊕.