Fig. 6.
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Evolution models of giant planets for three EOSs: SCvH95, CMS19, and our new EOS (CMS19 w/non-ideal effect), with Teq = 1500 K, taken at 4.5 Gyr. The models consist of a pure rocky core overlaid with a H-He envelope of solar composition. The coloured area for each EOS is bounded by evolution models without a core and with a 20 M⊕ core.
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