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Fig. 1


Relative populations xi = ni/nB for different stellar compositions: trapped matter with S/A = 2 (upper panels) or T = 40 MeV (central panels), and untrapped matter with T = 0 (lower panels). The GCN (left panels) or LCN (right panels) construction for the mixed phase is employed together with the MIT bag model for the quark phase.

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