Fig. 3.

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EOSs of β-stable neutrino-free matter at different temperature values of T = 0, 2, 5, 10, and 20 MeV. In the left panel, we use a cold crust assuming the transition between the cold crust and the uniform core fixed at n = 0.08 fm−3. In the right panel, we use a hot inner crust and the crust–uniform matter transition is determined as described in Sect. 3, consistently with Fig. 1.
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