出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：In the present work, we study some of the physical characteristics of neutron stars, especially the mass-radius relation and chemical compositions of the star within a relativistic model subject to a strong magnetic field. To study the influence of the magnetic field in the stellar interior, we consider altogether four solutions: two different values for the magnetic field to obtain a weak and a strong influence, and two configurations: a family of neutron stars formed only by protons, electrons and neutrons and another family formed by protons, electrons, neutrons, muons and hyperons. In both cases all the particles that constitutes the neutron star are in b equilibrium and the total net charge is zero.
