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arXiv · 0810.3390

Stellar matter with a strong magnetic field within density-dependent relativistic models

A. Rabhi·C. Providencia·J. Da Providencia
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Abstract

The effect of strong magnetic fields on the equation of state (EoS) for compact stars described with density-dependent relativistic hadronic models is studied. A comparison with other mean-field relativistic models is done. It is shown that the largest differences between models occur for low densities, and that the magnetic field affects the crust properties of a star, namely its extension.

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A. Rabhi, C. Providencia, J. Da Providencia. 2008-10-19. Stellar matter with a strong magnetic field within density-dependent relativistic models. https://doi.org/10.1088/0954-3899%2F35%2F12%2F125201

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