Three nominal models of Jupiter’s interior used in this study. The top panel shows the schematic models and the bottom panel shows the density (normalized by the density at the center) and the Brunt-Väisälä frequency (normalized by the dynamical frequency) as a function of the radius. The blue shadow in the bottom panel indicates solid regions. (a) A compact rigid core model; (b) an extended dilute core model; and (c) a compact rigid core and an outer stable layer model.