A model incorporating magnetic field decay and post-birth re-emergence explains why kinematic ages exceed characteristic ages in most magnetars.
Reality of inverse cascading in neutron star crusts.A&A2025,694, A39, [arXiv:astro- ph.HE/2408.08819]
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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.