A model incorporating magnetic field decay and post-birth re-emergence explains why kinematic ages exceed characteristic ages in most magnetars.
Hall effect in neutron star crusts: evolution, endpoint and dependence on initial conditions
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A phenomenological model of the magnetic field re-emergence in magnetars and discrepancy between the kinematic and characteristic ages
A model incorporating magnetic field decay and post-birth re-emergence explains why kinematic ages exceed characteristic ages in most magnetars.