Two-fluid CFL strange quark stars with scalar dark matter show non-monotonic maximum mass versus dark-matter mass and can occupy the lower mass gap while remaining qualitatively consistent with GW170817 tidal deformability.
Abbott et al., Astrophys
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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.
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Two fluid CFL strange quark stars with scalar dark matter: critical mass and mass gap implications
Two-fluid CFL strange quark stars with scalar dark matter show non-monotonic maximum mass versus dark-matter mass and can occupy the lower mass gap while remaining qualitatively consistent with GW170817 tidal deformability.
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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.