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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4 Pith papers cite this work, alongside 70 external citations. Polarity classification is still indexing.
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representative citing papers
Neutron star observations, especially the heaviest known pulsar masses and GW170817 tidal deformability, provide the strongest restrictions on the allowed cold dense matter equation of state.
Heavy-ion collision data and neutron-star observations yield consistent nuclear equations of state, with laboratory accuracy matching astronomical accuracy up to about 1.5 times nuclear saturation density.
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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Astrophysical constraints on the cold equation of state of the strongly interacting matter
Neutron star observations, especially the heaviest known pulsar masses and GW170817 tidal deformability, provide the strongest restrictions on the allowed cold dense matter equation of state.
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Nuclear equation-of-state at high density and multi-messenger astronomy: contribution of heavy-ion collisions
Heavy-ion collision data and neutron-star observations yield consistent nuclear equations of state, with laboratory accuracy matching astronomical accuracy up to about 1.5 times nuclear saturation density.
- On the Possibility of a Strong First-Order Phase Transition in Neutron Stars