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arXiv · 1411.7209

On Magnetized Neutron Stars

Luiz L. Lopes·Debora P. Menezes
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Abstract

In this work we review the formalism normally used in the literature about the effects of density-dependent magnetic fields on the properties of neutron and quark stars, expose some ambiguities that arise and propose a way to solve the related problem. Our approach explores more deeply the concept of pressure, yielding the so called chaotic magnetic field formalism for the stress tensor. We also use a different way of introducing a variable magnetic field, which depends on the energy density rather than on the baryonic density, which allows us to build a parameter free model.

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Luiz L. Lopes, Debora P. Menezes. 2015-08-05. On Magnetized Neutron Stars. https://doi.org/10.1088/1475-7516%2F2015%2F08%2F002

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