First-principles simulations find denser hydrogen at planetary conditions, implying lower bulk metallicity for Jupiter.
Note that the heavy-element mass fraction (i.e., the envelope metallicity) is assumed to be the same in the inner and outer envelopes
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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.