Self-consistent HFB calculations with Bloch boundary conditions show more than 90% of neutrons are superfluid in the inner crust crystal phase above 0.03 fm^{-3}, nearly independent of interaction and geometry details.
Superfluid extension of the self-consistent time-dependent band theory for neu- tron star matter: Anti-entrainment versus superfluid ef- fects in the slab phase
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Superfluid fraction in the crystal phase of the inner crust of neutron stars
Self-consistent HFB calculations with Bloch boundary conditions show more than 90% of neutrons are superfluid in the inner crust crystal phase above 0.03 fm^{-3}, nearly independent of interaction and geometry details.