Evolution of the inclination angle of radio pulsars is observable effect

摘要: It is shown that the slow glitches in spin rate of pulsar B1822-09 can be explained by reconstruction neutron star shape, which not matched with rotation axis. Owing to evolution inclination angle, i.e. angle between axis and magnetic dipole, under action braking torque, there appears disagreement symmetry After achieves maximum value alpha ~ 2x10^-4 shape becomes matching Such observed as glitch.