Investigation of the pulsars post-glitch relaxation in the context of inverse problem

The rotation of the neutron-proton vortex system in a neutron star with the pinning and depinning of the vortices is considered. Post-glitch relaxation solution of the equations of the dynamics of the pulsar rotation is compared with observational data of the pulsar Vela. It is shown that the relaxation parameters can be explained by the occurrence of 'density wave' of neutron vortices during the glitch, and features of the motion of vortices between two glitches