Samaddar, S. K.De, J. N.Viñas Gausí, XavierCentelles Aixalà, Mario2013-08-302013-08-3020090556-2813https://hdl.handle.net/2445/45448The 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.11 p.application/pdfeng(c) American Physical Society, 2009SupernovesConstitució de la matèriaFísica nuclearAstrofísicaSupernovaeConstitution of matterNuclear physicsAstrophysicsinfo:eu-repo/semantics/article5697962013-08-30info:eu-repo/semantics/openAccess