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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A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.
A pedagogical review of lattice QCD results on the thermodynamics of hot, dense, and magnetized QCD matter with an outlook on open questions.
citing papers explorer
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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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Chiral, parity-doublet, effective-Lagrangian mean-field theories for nuclear and astrophysical phenomenology
A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.
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Thermodynamics of magnetized matter in hot and dense QCD
A pedagogical review of lattice QCD results on the thermodynamics of hot, dense, and magnetized QCD matter with an outlook on open questions.