The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars

Figure 6

The equation of state for Λ from (𝑛,𝑝,𝑒) to (𝑛,𝑝,Λ,𝑒). The EOS for 𝑟^𝜎_Λ𝑁=1/3 becomes softer in (𝑛,𝑝,Λ,𝑒) phase.