Bayesian analysis of a smooth hadron-quark crossover EOS finds current observations tightly constrain the density dependence of nuclear symmetry energy while leaving highest-density hadronic and quark-matter parameters only weakly constrained.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.
citing papers explorer
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Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover
Bayesian analysis of a smooth hadron-quark crossover EOS finds current observations tightly constrain the density dependence of nuclear symmetry energy while leaving highest-density hadronic and quark-matter parameters only weakly constrained.
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Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective
Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.