Magnetized Neutron Stars

Gibran H. de Souza, Ernesto Kemp, Cecilia Chirenti
2017 International Journal of Modern Physics, Conference Series  
In this work we show the results for numerical solutions of the relativistic Grad-Shafranov equation for a typical neutron star with 1.4 solar masses. We have studied the internal magnetic field considering both the poloidal and toroidal components, as well as the behavior of the field lines parametrized by the ratio between these components of the field.
doi:10.1142/s2010194517600321 fatcat:czhx3lojjjedlj47b2sg6x4xxa