New phenomenological anisotropy profiles in hybrid stars, driven by superconductivity and magnetic fields, lead to enhanced masses and continuous gravitational wave emission.
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In the modified NJL model, low vacuum pressure with a first-order chiral transition supports massive non-strange quark stars consistent with pulsar data while high vacuum pressure with crossover is ruled out, constraining current quark mass to 4.08-4.13 MeV and suggesting GW170817 could involve such
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Anisotropic hybrid stars: Interplay of superconductivity and magnetic field leading to gravitational waves
New phenomenological anisotropy profiles in hybrid stars, driven by superconductivity and magnetic fields, lead to enhanced masses and continuous gravitational wave emission.
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QCD vacuum pressure and its influence on the equation of state of non-strange quark stars
In the modified NJL model, low vacuum pressure with a first-order chiral transition supports massive non-strange quark stars consistent with pulsar data while high vacuum pressure with crossover is ruled out, constraining current quark mass to 4.08-4.13 MeV and suggesting GW170817 could involve such