Explosive reconnection in magnetars
arXiv:astro-ph/0303384 · doi:10.1046/j.1365-2966.2003.07110.x
Abstract
X-ray activity of Anomalous X-ray Pulsars and Soft Gamma-Ray Repeaters may result from the heating of their magnetic corona by direct currents dissipated by magnetic reconnection. We investigate the possibility that X-ray flares and bursts observed from AXPs and SGRs result from magnetospheric reconnection events initiated by development of tearing mode in magnetically-dominated relativistic plasma. We formulate equations of resistive force-free electrodynamics, discuss its relation to ideal electrodynamics, and give examples of both ideal and resistive equilibria. Resistive force-free current layers are unstable toward the development of small-scale current sheets where resistive effects become important. Thin current sheets are found to be unstable due to the development of resistive force-free tearing mode. The growth rate of tearing mode is intermediate between the short \Alfven time scale and a long resistive time scale : , similar to the case of non-relativistic non-force-free plasma. We propose that growth of tearing mode is related to the typical rise time of flares, msec. Finally, we discuss how reconnection may explain other magnetar phenomena and ways to test the model.
27 pages, 3 figures, submitted to MNRAS
References in corpus (4)
Cited by in corpus (179)
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