RMF-CC models with ωρ coupling better match multi-messenger NS data and LQCD/NEP constraints than the baseline, yet standard RMF remains preferred without core phase transitions, requiring high Ksat ~300 MeV.
Lindblom, Phys
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Mass-gap compact objects (2.5–5 M☉) can be modeled as neutron stars within f(R,T)=R+2λT gravity using the AV18 equation of state with Bowers-Liang anisotropy and strong magnetic fields.
citing papers explorer
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Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations
RMF-CC models with ωρ coupling better match multi-messenger NS data and LQCD/NEP constraints than the baseline, yet standard RMF remains preferred without core phase transitions, requiring high Ksat ~300 MeV.
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Structure of Anisotropic Magnetized Neutron Stars in f(R,T) Gravity with Realistic Equation of State
Mass-gap compact objects (2.5–5 M☉) can be modeled as neutron stars within f(R,T)=R+2λT gravity using the AV18 equation of state with Bowers-Liang anisotropy and strong magnetic fields.