期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 322, 期 1-4, 页码 129-133出版社
SPRINGER
DOI: 10.1007/s10509-008-9958-5
关键词
Equation of state; First-principles simulations; Density functional theory; Hydrogen-helium mixtures; Giant planet interiors
资金
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [0813934] Funding Source: National Science Foundation
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, the groups derived very different conclusions. In particular estimates for the size of Jupiter's core and the metallicity of its hydrogen-helium mantle differed substantially. In this paper, we discuss the differences of the approaches and give an explanation for the differing conclusions.
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