First-principles simulations find denser hydrogen at planetary conditions, implying lower bulk metallicity for Jupiter.
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Applies Yukhnovskii-Kelbg methods to electrolytes and high-T plasmas, predicting density-driven transition to oscillating correlations and thermodynamic scaling shifting from n^{1/2} to n^{1/4} while respecting the Onsager bound.
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A Denser Hydrogen Inferred from First-Principles Simulations Challenges Jupiter's Interior Models
First-principles simulations find denser hydrogen at planetary conditions, implying lower bulk metallicity for Jupiter.