Physical Review Letters · 1997 · 245 citations · 34 references
EngineeringNuclear PhysicsPhysicsHigh-energy Nuclear ReactionNatural SciencesApplied PhysicsNeutron SourceNuclear Symmetry EnergyNuclear Many-body PhysicsShort-range CorrelationsAsymmetric Nuclear MatterNeutron ScatteringPre-equilibrium NeutronsNeutron-rich NucleiSymmetric Nuclear Matter
The ratio of pre-equilibrium neutrons to protons from collisions of neutron-rich nuclei is studied as a function of their kinetic energies. This ratio is found to be sensitive to the density dependence of the nuclear symmetry energy, but is independent of the compressibility of symmetric nuclear matter and the in-medium nucleon-nucleon cross sections. The experimental measurement of this ratio thus provides a novel means for determining the nuclear equation of state of asymmetric nuclear matter.
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Equation of state for dense nucleon matter
R. B. Wiringa, V. B. Fiks, A. Fabrocini · Physical Review C · 1988 · 947 citations
Direct URCA process in neutron stars
James M. Lattimer, C. J. Pethick, Madappa Prakash et al. · Physical Review Letters · 1991 · 772 citations
Direct Urca Process, Neutron Star Physics, High-energy Nuclear Reaction +8