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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
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Review of heavy-ion collision constraints on the nuclear EoS that produce neutron-star pressure profiles consistent with gravitational-wave and pulsar observations up to 2.5 n_sat.
citing papers explorer
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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.
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Nuclear equation-of-state at high density and multi-messenger astronomy: contribution of heavy-ion collisions
Review of heavy-ion collision constraints on the nuclear EoS that produce neutron-star pressure profiles consistent with gravitational-wave and pulsar observations up to 2.5 n_sat.