Magnetic-field evolution in a plastically failing neutron-star crust

ABSTRACT Under normal conditions in a neutron-star (NS) crust, ions are locked in place in the crustal lattice and only electrons are mobile, and magnetic-field evolution is thus directly related to the electron velocity. The evolution, however, builds magnetic stresses that can become sufficiently...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2019-07, Vol.486 (3), p.4130-4143
Hauptverfasser: Lander, S K, Gourgouliatos, K N
Format: Artikel
Sprache:eng
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