Symmetry coefficients and incompressibility of clusterized supernova matter

Details Symmetry coefficients and incompressibility of clusterized supernova matter Symmetry coefficients and incompressibility of clusterized supernova matter

2009-06-26

arxiv.org/abs/0906.4909v1

Phys.Rev.C80:035803,2009

Physics

Nuclear Physics

Nuclear Theory

9 pages + 12 figures

Scientific paper

10.1103/PhysRevC.80.035803

The symmetry energy coefficients, incompressibility, and single-particle and isovector potentials of clusterized dilute nuclear matter are calculated at different temperatures employing the $S$-matrix approach to the evaluation of the equation of state. Calculations have been extended to understand the aforesaid properties of homogeneous and clusterized supernova matter in the subnuclear density region. Comparison of the results in the $S$-matrix and mean-field approach reveals some subtle differences in the density and temperature region we explore.

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