Vector interactions enlarge anisotropic surface tension of quark matter in magnetic fields, cause transverse tension to rise with B in strong fields, require moderate B for bubble formation, and slightly reduce stability.
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Quark stars in Ricci-Determinant gravity with interacting quark EoS exhibit lower compactness than in GR and become unstable at high central densities when perturbative gravity terms exceed about half the GR contribution.
citing papers explorer
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Anisotropic surface tension and stability of quark matter modified by the vector interaction
Vector interactions enlarge anisotropic surface tension of quark matter in magnetic fields, cause transverse tension to rise with B in strong fields, require moderate B for bubble formation, and slightly reduce stability.
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Quark Stars in Ricci-Determinant Gravity with an Interacting Quark Equation of State
Quark stars in Ricci-Determinant gravity with interacting quark EoS exhibit lower compactness than in GR and become unstable at high central densities when perturbative gravity terms exceed about half the GR contribution.