Fig. G.1
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Planetary radius vs. time for the models with a wide composition gradient and warm initial conditions. The solid and dashed line correspond to the CMS and SCvH EoS for Η-He, respectively. The colors, blue, green and red show different planetary masses of Mp =5, 10, and 15Μ⊕, respectively. For each simulations we show the radius after t = 10 Gyr on the right hand side.
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