Plastic damping of Alfvén waves in magnetar flares and delayed afterglow emission
arXiv:1505.03465 · doi:10.1088/0004-637X/815/1/25
Abstract
Magnetar flares generate Alfvén waves bouncing in the closed magnetosphere with energy up to erg. We show that on a 10-ms timescale the waves are transmitted into the star and form a compressed packet of high energy density. This packet strongly shears the stellar crust and initiates a plastic flow, heating the crust and melting it hundreds of meters below the surface. A fraction of the deposited plastic heat is eventually conducted to the stellar surface, contributing to the surface afterglow months to years after the flare. A large fraction of heat is lost to neutrino emission or conducted into the core of the neutron star.
10 pages, 12 figures, submitted to ApJ
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