Fig. 1

Dependence of the critical unpairing field Hc2 on baryonic density (solid line). The density is normalized to the nuclear saturation density n0 = 0.16 fm-3 and the equation of state and composition of matter is the same as in Sinha & Sedrakian (2015a). This arrangment of flux-free and flux-featuring phases arises in the case of intermediate field magnetars with average constant field B<Hc2, which is indicated by the dashed line.
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