2008/10/01 by A. Rabhi, A Rabhi, C. Providencia +3 · 61 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #Equation of state #Field (mathematics) #Magnetic field #Pulsars and Gravitational Waves Research #Relativistic beaming #Relativistic particle #Relativistic quantum chemistry #Stars #astro-ph #nucl-th
paper · pdf · doi:10.1088/0954-3899/35/12/125201
published in Journal of Physics G Nuclear and Particle Physics 35(12), 125201 (IOP Publishing) · 21 pages, 10 figures and 2 tables
openalex publication_date 2008/10/01 · arxiv created 2008/10/19 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
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.