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

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.

21 pages, 10 figures and 2 tables

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Cited by in corpus (46)

• Equation of State of a Dense and Magnetized Fermion System
• Quark matter under strong magnetic fields in the Nambu--Jona-Lasinio Model
• Consistent neutron star models with magnetic field dependent equations of state
• Bulk Properties of a Fermi Gas in a Magnetic Field
• Equation of state for the MCFL phase and its implications for compact star models
• Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
• Heavy Baryons in Compact Stars
• The pasta phase within density dependent hadronic models
• Quark-hadron phase transition in a neutron star under strong magnetic fields
• (In-)Significance of the Anomalous Magnetic Moment of Charged Fermions for the Equation of State of a Magnetized and Dense Medium
• The influence of strong magnetic fields on proto-quark stars
• Hypernuclear matter in strong magnetic field
• Quark-gluon plasma in an external magnetic field
• Hadronic and hybrid stars subject to density dependent magnetic fields
• Magnetic effects in heavy-ion collisions at intermediate energies
• Nuclear structure in strong magnetic fields: nuclei in the crust of a magnetar
• Neutron Stars with Hyperons subject to Strong Magnetic Field
• Deformation of a magnetized neutron star
• Magnetism in Dense Quark Matter
• Warm and dense stellar matter under strong magnetic fields
• Thermodynamics of Neutrons in a Magnetic Field and its Implications for Neutron Stars
• Equation of state of strongly magnetized matter with hyperons and $\Delta$-resonances
• Heavy Magnetic Neutron Stars
• Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field
• Dense stellar matter with trapped neutrinos under strong magnetic fields
• Magnetization of neutron star matter
• Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
• Thermodynamic Behaviour of Magnetized QGP within the Self-Consistent Quasiparticle Model
• Quark matter under strong magnetic fields
• Is the magnetic field making the inner crust of neutron stars more heterogeneous?
• Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields
• Dense nuclear matter and symmetry energy in strong magnetic fields
• Structure of ultra-magnetised neutron stars
• Spinodal instabilities and the distillation effect in nuclear matter under strong magnetic fields
• Thermomagnetic properties and Debye Screening for magnetized quark-gluon Plasma using the extended self-consistent quasiparticle model
• Effect of the $\delta$-meson on the instabilities of nuclear matter under strong magnetic fields
• Magnetic-Field Induced Deformation in Hybrid Stars
• Temperature and Strong Magnetic Field Effects in Dense Matter
• Landau parameters for asymmetric nuclear matter with a strong magnetic field
• Magnetised neutron star crust within effective relativistic mean-field model
• Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields
• Pasta phases in neutron stars under strong magnetic fields
• Strong magnetic fields: neutron stars with an extended inner crust
• Properties of strongly magnetized ultradense matter and their imprints on magnetar pulsations
• Strongly interacting matter in extreme magnetic fields
• Effects of anisotropy on strongly magnetized neutron and strange quark stars in general relativity