Fig. 16.

Upper panel: heat capacity per one baryon in units of kB as a function of density in the partially accreted inner crust at T = 108 K. Partial contributions from the nuclei (dotted line), electrons (dot-dashed lines), dripped neutrons (short-dashed line), and dripped protons (long-dashed line), as well as their sum (solid line) are shown. Lower panel: critical temperatures of superfluidity of neutrons (short-dashed lines) and protons (long-dashed lines), and the ion plasma temperature (dotted line).
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