For the TW99 model at entropy per baryon S=1 and lepton fraction YL=0.4, adding σ* and φ mesons shifts the moment-of-inertia peak to higher density, slightly reduces its height, and lowers I by about 0.6% only near 2.7 solar masses.
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Does strange meson condensation reduce the moment of inertia of massive proto neutron stars? insights at S = 1 and YL = 0.4
For the TW99 model at entropy per baryon S=1 and lepton fraction YL=0.4, adding σ* and φ mesons shifts the moment-of-inertia peak to higher density, slightly reduces its height, and lowers I by about 0.6% only near 2.7 solar masses.