作者: W. B. Hubbard , B. Militzer
DOI: 10.1007/S10509-008-9958-5
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摘要: Recently two groups used first-principles computer simulations to model Jupiter’s interior. While both studies relied on the same simulation technique, density functional molecular dynamics, derived very different conclusions. In particular estimates for size of core and metallicity its hydrogen-helium mantle differed substantially. this paper, we discuss differences approaches give an explanation differing