Unified AMD analysis constrains nuclear symmetry energy at 0.28 saturation density to 13.84 ± 1.31 MeV via combined neutron-skin and dipole polarizability data.
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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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Revisiting neutron-skin thickness and dipole polarizability constraints on the symmetry energy in Antisymmetrized Molecular Dynamics
Unified AMD analysis constrains nuclear symmetry energy at 0.28 saturation density to 13.84 ± 1.31 MeV via combined neutron-skin and dipole polarizability data.
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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.