Gravitational radiation from neutron stars deformed by crustal Hall drift

A precondition for the radio emission of pulsars is the existence of strong, small-scale magnetic field structures (‘magnetic spots’) in the polar cap region. Their creation can proceed via crustal Hall drift out of two qualitatively and quantitatively different initial magnetic field configurations...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-07, Vol.459 (3), p.3407-3418
Hauptverfasser:	Suvorov, A. G., Mastrano, A., Geppert, U.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Deformation mechanisms Drift Field strength Gravitational waves Magnetic fields Neutron stars Pulsars Radio astronomy Spots Star & galaxy formation Stars
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