Magnetized Neutron Stars
Gibran H. de Souza, Ernesto Kemp, Cecilia Chirenti
TL;DR
This paper presents numerical solutions to the relativistic Grad-Shafranov equation for neutron stars, analyzing their internal magnetic fields with combined poloidal and toroidal components and field line behavior.
Contribution
It provides the first detailed numerical analysis of the internal magnetic field configurations in relativistic neutron stars considering both field components.
Findings
Numerical solutions for magnetic field configurations in neutron stars.
Analysis of the ratio between poloidal and toroidal magnetic components.
Insights into the behavior of magnetic field lines within neutron stars.
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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