Comparison of Jupiter Interior Models Derived from First-Principles Simulations

Abstract

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.

5 pages, no figures

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Cited by in corpus (10)

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• Anelastic tidal dissipation in multi-layer planets
• Jupiter internal structure: the effect of different equations of state
• Frontiers of the physics of dense plasmas and planetary interiors: experiments, theory, applications
• Temperature-Dependent Behavior of Confined Many-electron Systems in the Hartree-Fock Approximation
• Quantum Langevin molecular dynamics determination of the solar-interior equation of state
• Predictions on the core mass of Jupiter and of giant planets in general
• Magnesium Oxide at Extreme Temperatures and Pressures Studied with First-Principles Simulations
• Study of Jupiter's Interior with Quadratic Monte Carlo Simulations