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Magnetized Neutron Stars

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arxiv 1910.06263 v1 pith:SILFWRKY submitted 2019-10-14 astro-ph.HE

Gibran H. de Souza , Ernesto Kemp , Cecilia Chirenti This is my paper · ORCID
classification astro-ph.HE
keywords fieldcomponentsneutronbehaviorconsideringequationgrad-shafranovinternal
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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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Cited by 1 Pith paper

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  1. New Universal Relations for Magnetized Neutron Stars

    gr-qc 2026-08 conditional novelty 7.0 of 10

    Magnetized neutron stars with dipole fields obey a new exact relation between dipole moment and compactness, and approximate EoS-insensitive relations among dipole moment, quadrupole moment, and ellipticity.

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