arXiv · nucl-th/0605002
Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
Abstract
It is shown that the experimentally observed decrease of the nuclear symmetry energy with the increasing centrality or the excitation energy in isotopic scaling analyses of heavy-ion reactions can be well understood analytically within a degenerate Fermi gas model. The evolution of the symmetry energy is found to be mainly due to the variation in the freeze-out density rather than temperature. The isoscaling analyses are useful for probing the interaction part of the nuclear symmetry energy, provided that both the freeze-out temperature and density of the fragments can be inferred simultaneously from the experiments.
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Bao-An Li, Lie-Wen Chen. 2006-08-31. Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions. https://doi.org/10.1103/physrevc.74.034610
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