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arXiv · 1910.06263

Magnetized Neutron Stars

Gibran H. de Souza·Ernesto Kemp·Cecilia Chirenti
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Abstract

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.

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Gibran H. de Souza, Ernesto Kemp, Cecilia Chirenti. 2019-10-14. Magnetized Neutron Stars. https://doi.org/10.1142/s2010194517600321

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