Light clusters as a possible source of crustal impurities: A quasi-particle approach

Open Access

Fig. 6.

Impurity parameter, Q_imp, as a function of the total baryon density, ρ, in a CLD calculation with five light clusters for all models considered in this work in β equilibrium and at T = 1 MeV (top panel), T = 0.5 (middle panel), and at the crystallization temperature, T_melt (bottom panel). Results were obtained employing the corrected translational free energy, $F_{trans}^{★}$ $F^{\star }_{\mathrm {trans}}$ .

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