paper

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

References in corpus (13)

Cited by in corpus (29)