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From crystalline to exotic arrangements of matter in neutron star crusts

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Figure

Table 1: Synopsis of basic Euler characteristic values.
Figure 1: (Colour on line) Time evolution of neutron density in oxygen SCC latticewith xp=0.1, ⟨ρ⟩=0.0726 fm−3 and threshold density 0.065 fm−3.
Figure 3: (Colour online) Snapshots of neutron density at t=600 fm/c in perturbedoxygen SCC lattice with ⟨ρ⟩=0.06 fm−3 for (a) xp=0.5 and (b) xp=0.2.
Figure 5: Structure diagram corresponding to the system in Fig. 4.

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