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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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SAMADDAR, S. K., et al. Symmetry coefficients and incompressibility of clusterized supernova matter. Physical Review C. 2009. Vol. 80, num. 3, pags. 035803-1-035803-11. ISSN 0556-2813. [consulted: 18 of October of 2026]. Available at: https://hdl.handle.net/2445/45448