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.
(9), obtaining quasi-particle energiesE α(pb) and eigenvectors (U ∗ αn(pb),−V ∗ αn(pb))
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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.