Figure 24: Baryon chemical potential at , vs. pressure for different
models of neutron star crust. Black solid line: for the ground-state crust. Lines with
discontinuous drops: for four evolution models in the accreted crust with . Upper
four smooth lines, which nearly coincide: . For an explanation see
the text. Based on Haensel & Zdunik [188]. Figure made by J.L. Zdunik.
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