We show that the crust-core interface in neutron stars acts as a potential
barrier to the peripheral neutron vortices approaching the interface in the
model in which these are coupled to the proton vortex clusters. This elementary
barrier because of the interaction of vortex magnetic flux with the Meissner
currents set up by the crustal magnetic field at the interface. The dominant
part of the force is derived from to the cluster-interface interaction. As a
result of the stopping of the continuous neutron vortex current through the
interface, angular momentum is stored in the superfluid layers in the vicinity
of the crust-core interface during the interglitch period. Discontinuous
annihilation of proton vortices on the boundary restores the neutron vortex
current and spins up the observable crust on short time-scales, leading to a
glitch in the spin characteristics of a pulsar.Comment: 12 pages, 3 figures. Final version to appear in MNRAS; includes a new
discussion of the problem in the spherical geometry; some rewording;
references revise