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An internal mechanism for the anti-glitch observed in AXP 1E 2259+586

Magnetars are fascinating objects that are thought to be neutron stars powered by their strong internal magnetic fields. Clear evidence of a sudden spin-down was detected in the Anomalous X-ray Pulsar AXP 1E 2259+586, an object cataloged as a magnetar. This event received the name "anti-glitch". In this work we present a simple internal mechanism which could account for the observed sudden spin-down of the star.

preprint2015arXivOpen access
Ignacio F. Ranea-SandovalFederico García
astro-ph.HE
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Ignacio F. Ranea-SandovalFederico García

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