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

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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.
21 pages, 10 figures and 2 tables

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Nuclear Theory, Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/172363

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0810.3390
 http://arxiv.org/abs/0810.3390
 J. Phys. G: Nucl. Part. Phys. 35, 125201 (2008)
 doi:10.1088/0954-3899/35/12/125201

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