Fig. 11.
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Evolution of the gray opacity κgray for a sampling of fluid elements across all angles and depths, from simulations using different opacity models. Top row: Runs using the analytical expression from Wu et al. (2022, left) or the prescription from Just et al. (2022, right). Central row: Simulations with Rosseland (left) or Planck (right) gray opacities computed from the LANL data for neodymium as representative of the lanthanides. Bottom row: Rosseland mean opacity from the multigroup models using only neodymium to represent lanthanides (left) or also uranium as representative of actinides (right). The color bar is cut at κgray = 10−2 cm2g−1 for easier visualization. For each simulation, the top and bottom subpanels show the trajectories of the fluid elements in the density-temperature and density-cumulative lanthanides mass fraction (Xlan) planes, respectively. Markers indicate different orders of magnitudes of Xlan, with circles for Xlan < 5 × 10−5, downward triangles for 10−5 < Xlan < 10−3, upward triangles for 10−3 < Xlan < 5 × 10−2, and stars for Xlan > 5 × 10−2. For the simulations using only neodymium data, the background shows the single-element mean opacity κel calculated from the LANL tables (Rosseland for GK and Nd300, Planck for GKPl). Similarly, the uranium Rosseland mean opacity is shown in the NdU300 panel.
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