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

Open Access

Fig. 5.

Mass fractions of light clusters (top panel), heavy clusters (middle panel), and unbound nucleons (bottom panel) as a function of the total baryon density, ρ, in the inner crust at T = 1 MeV for all models considered in this work. The results were obtained employing the corrected translational free energy, $F_{trans}^{★}$ $F^{\star }_{\mathrm {trans}}$ .

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