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Accurate nuclear symmetry energy at finite temperature within a BHF approach

We compute the free energy of asymmetric nuclear matter in a Brueckner-Hartree-Fock approach at finite temperature, paying particular attention to the dependence on isospin asymmetry. The first- and second-order symmetry energies are determined as functions of density and temperature and useful parametrizations are provided. We find small deviations from the quadratic isospin dependence and very small corresponding effects on (proto)neutron star structure.

preprint2020arXivOpen access
Jia-Jing LuFan LiZeng-Hua LiChong-Yang ChenG. F. BurgioH. -J. Schulze
nucl-th
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Open access6 authors1 topic
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Jia-Jing LuFan LiZeng-Hua LiChong-Yang ChenG. F. BurgioH. -J. Schulze

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