Temperature dependence of nuclear matter generalized isovector symmetry energy with Skyrme-type interactions
F. L. Braghin

TL;DR
This study examines how the isovector symmetry energy coefficient in nuclear matter varies with temperature using Skyrme interactions, revealing minimal temperature dependence but parameter-dependent behaviors at sub-saturation densities.
Contribution
It provides a detailed analysis of the temperature dependence of the symmetry energy coefficient within the Skyrme framework, highlighting the influence of different parameterizations.
Findings
Temperature variation of $\\cA_{0,1}$ is minimal (around 1 MeV) up to 18 MeV.
Behavior of $\\cA_{0,1}$ with temperature depends on Skyrme parameters.
Significant differences occur at densities below saturation density.
Abstract
The temperature dependence of the nuclear matter isovector symmetry energy coefficient () is investigated in the framework of the generalized nuclear polarizability with Skyrme interactions, as worked out in Refs. \cite{npa,prc}. The variation of is very small (of the order of 1 MeV) for temperatures (T) in the range of 0 and 18 MeV. Different behaviors with temperature are found strongly depending on the Skyrme parameterization, in particular at densities lower than the saturation density .
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