]>The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars : Figure 8
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Figure 8: Nucleon symmetry energies of (n,p,e), (n,p,Σ,e), and (n,p,Λ,e) are shown with the solid, doted, and dot-dashed lines, respectively. The ratios of hyperon coupling constants are rΣNσ=1.0 and rΛNσ=1.0. The discontinuity of symmetry energy, (n,p,Σ,e), occurs at ρB/ρ0~3.641, because of the phase transition from (n,p,Σ,e) to (n,p,Σ).