Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.
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Three-dimensional band-structure calculations in the BCS approximation within HFB theory find that only 8% of free neutrons participate in superflow at baryon density 0.03 fm^{-3}, independent of the pairing gap.
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Superfluid fraction and effective ion mass in the crystalline crust of a neutron star: role of interband response
Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.