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Symmetry coefficients and incompressibility of clusterized supernova matter

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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. A 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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Articles publicats en revistes (Física Quàntica i Astrofísica)

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Symmetry coefficients and incompressibility of clusterized supernova matter