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

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dc.creatorRabhi, A.
dc.creatorProvidencia, C.
dc.creatorDa Providencia, J.
dc.date2008-10-19
dc.date.accessioned2026-07-07T10:12:57Z
dc.date.available2026-07-07T10:12:57Z
dc.descriptionThe 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.
dc.description21 pages, 10 figures and 2 tables
dc.identifierhttps://arxiv.org/abs/0810.3390
dc.identifierhttp://arxiv.org/abs/0810.3390
dc.identifierJ. Phys. G: Nucl. Part. Phys. 35, 125201 (2008)
dc.identifierdoi:10.1088/0954-3899/35/12/125201
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/172363
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleStellar matter with a strong magnetic field within density-dependent relativistic models
dc.typetext

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