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A region of toroidally oriented quantized flux lines must exist in the protonsuperconductor in the core of the neutron star. This region will be a site ofvortex pinning and creep. Entrainment of the neutron superfluid with thecrustal lattice leads to a requirement of superfluid moment of inertiaassociated with vortex creep in excess of the available crustal moment ofinertia. This will effect constraints on the equation of state. The toroidalflux region provides the moment of inertia necessary to complement the crustsuperfluid with postglitch relaxation behavior fitting the observations.

Vortex Creep Against Toroidal Flux Lines, Crustal Entrainment, and Pulsar Glitches