Simulation Results for the paper: Core-Envelope Miscibility in Sub-Neptunes and Super-Earths

Results of ab initio simulations using the phase-coexistence method (EDTable 1) and of homogeneous simulations (EDTable 2) as described in: "Core-Envelope Miscibility in Sub-Neptunes and Super-Earths" by Gilmore and Stixrude.采用相共存法（phase-coexistence method，EDTable 1）与均匀态模拟（homogeneous simulations，EDTable 2）完成的从头算模拟（ab initio simulations）结果，如吉尔莫尔与施特克斯鲁德在论文《亚海王星与超级地球的核幔混合性》中所述。