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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2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
Hybrid star models with constant sound speed quark matter match NICER data for PSR J0740+6620 and PSR J0030+0451 only when the energy density discontinuity at the phase transition is small and the quark sound speed is relatively high.
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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Can a hybrid star with constant sound speed parametrization explain the new NICER mass-radius measurements ?
Hybrid star models with constant sound speed quark matter match NICER data for PSR J0740+6620 and PSR J0030+0451 only when the energy density discontinuity at the phase transition is small and the quark sound speed is relatively high.