Simultaneous Evolutionary Fits for Jupiter and Saturn Incorporating Fuzzy Cores
Ankan Sur, Roberto Tejada Arevalo, Yubo Su, Adam Burrows

TL;DR
This paper develops non-adiabatic evolutionary models for Jupiter and Saturn with fuzzy cores, successfully fitting key observables and revealing insights into their internal structure and composition, including helium distribution and heavy-element content.
Contribution
It introduces simultaneous evolutionary models for both planets incorporating fuzzy cores and non-adiabatic processes, advancing understanding of their internal structures.
Findings
Models fit observed bulk properties of Jupiter and Saturn.
Fuzzy cores are preserved from birth, requiring lower initial entropies.
Predicted atmospheric helium fraction for Saturn is ~0.2.
Abstract
With the recent realization that there likely are stably-stratified regions in the interiors of both Jupiter and Saturn, we construct new non-adiabatic, inhomogeneous evolutionary models with the same microphysics for each that result at the present time in respectable fits for all major bulk observables for both planets. These include the effective temperature, radius, atmospheric heavy-element and helium abundances (including helium rain), and the lower-order gravity moments J2 and J4. The models preserve from birth most of an extended "fuzzy" heavy-element core. Our predicted atmospheric helium mass fraction for Saturn is ~0.2, close to some measured estimates, but in disagreement with some published predictions. To preserve a fuzzy core from birth, the interiors of both planets must start out at lower entropies than would be used for traditional "hot start" adiabatic models, though…
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Taxonomy
TopicsFuzzy Logic and Control Systems · Metaheuristic Optimization Algorithms Research · Evolutionary Algorithms and Applications
