A model incorporating magnetic field decay and post-birth re-emergence explains why kinematic ages exceed characteristic ages in most magnetars.
Initial spin periods of neutron stars in supernova remnants.Astroph.Sp.Sci.2012,341, 457–464, [arXiv:astro-ph.HE/1204.0632]
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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.