Abstract
The magnetized vortex lines of the 3 P 2 paired neutron superfluid are effectively pinned by the magnetic energy barriers produced by the flux tubes of the 1 S 0 paired proton superconducting fluid. The stellar crust and the core superfluid can be coupled primarily via thermal vortex creep against the barriers. The postglitch relaxation of the core superfluid is studied by using the thermal vortex creep model in the limit where the motion of flux tubes is slow compared with that of the vortex lines
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