Recognition: unknown
Hall Equilibria: Solutions with toroidal and poloidal magnetic fields in Neutron Star Crusts
classification
🌌 astro-ph.SR
keywords
crustshallmagneticneutronpoloidalsolutionstoroidalanalytically
read the original abstract
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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.