Neutron star deformation due to poloidal–toroidal magnetic fields of arbitrary multipole order: a new analytic approach
A recipe is presented to construct an analytic, self-consistent model of a non-barotropic neutron star with a poloidal-toroidal field of arbitrary multipole order, whose toroidal component is confined in a torus around the neutral curve inside the star, as in numerical simulations of twisted tori. T...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2015-03, Vol.447 (4), p.3475-3475 |
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Sprache: | eng |
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