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arxiv: 1305.0149 · v1 · pith:UTCL6OYOnew · submitted 2013-05-01 · 🌌 astro-ph.SR

Hall Equilibria: Solutions with toroidal and poloidal magnetic fields in Neutron Star Crusts

classification 🌌 astro-ph.SR
keywords crustshallmagneticneutronpoloidalsolutionstoroidalanalytically
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We present Hall equilibrium solutions for neutron stars crusts containing toroidal and poloidal magnetic field. Some simple cases are solved analytically while more complicated configurations are found numerically through a Gauss-Seidel elliptic partial differential equation solver.

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