Fig. 5.
Gibbs free energy per nucleon g in accreting NS crust and catalysed NS crust (thin bottom lines). Top panel: predictions from the model of MB and from the model based on the BSk19 EDF comparing two different treatments for the inner crust: ETFSI vs. ETF (no shell correction). Bottom panel: predictions from models based on differents EDFs. See text for details.
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