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.
B.et al.Isospin diffusion and the nuclear symmetry energy in heavy ion reactions.Phys
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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.