Stellar matter with a strong magnetic field within density-dependent relativistic models
Nuclear Theory
2008-10-27 v1 Astrophysics
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.
Cite
@article{arxiv.0810.3390,
title = {Stellar matter with a strong magnetic field within density-dependent relativistic models},
author = {A. Rabhi and C. Providencia and J. Da Providencia},
journal= {arXiv preprint arXiv:0810.3390},
year = {2008}
}
Comments
21 pages, 10 figures and 2 tables