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

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

2008-10-19

arxiv.org/abs/0810.3390v1

J. Phys. G: Nucl. Part. Phys. 35, 125201 (2008)

Physics

Nuclear Physics

Nuclear Theory

21 pages, 10 figures and 2 tables

Scientific paper

10.1088/0954-3899/35/12/125201

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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