Her X-1 precession implies unpinned crustal superfluid vortices with weak mutual friction persisting for centuries.
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Mean-field theory extended to unequal critical temperatures shows neutron vortex cores exceed magnetic penetration depth in neutron star outer cores.
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Theoretical Constraints on Neutron Star Superfluidity from Her X-1 Precession
Her X-1 precession implies unpinned crustal superfluid vortices with weak mutual friction persisting for centuries.
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The mean-field theory of superfluid-superconducting vortex states in the outer core of neutron stars
Mean-field theory extended to unequal critical temperatures shows neutron vortex cores exceed magnetic penetration depth in neutron star outer cores.