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- W2133921977 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." @default.
- W2133921977 created "2016-06-24" @default.
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- W2133921977 date "2015-08-03" @default.
- W2133921977 modified "2023-10-17" @default.
- W2133921977 title "On magnetized neutron stars" @default.
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- W2133921977 doi "https://doi.org/10.1088/1475-7516/2015/08/002" @default.
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