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Stellar matter with a strong magnetic field within density-dependent relativistic models
Authors: A. Rabhi, C. Providência and J. Da Providência
Ref.: J. Phys. G: Nucl. Part. Phys. 35, 125201-1-125201-17 (2008)
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.
