The iterative method recently proposed for determining the internal constitution of the outer crust of a nonaccreted neutron star is extended to magnetars by taking into account the Landau-Rabi quantization of electron motion induced by the presence of a very high magnetic field. It is shown that in the strongly quantizing regime, the method can be efficiently implemented using new analytical solutions for the transitions between adjacent crustal layers. Detailed numerical computations are performed to assess the performance and precision of the method.info:eu-repo/semantics/publishe
International audienceIn this review we discuss self-consistent methods to calculate the global stru...
We have studied various physical properties of magnetically deformed atoms and the associated matter...
Isolated neutron stars show a diversity in timing and spectral properties, which has historically le...
This computer code (written in C language) determines the internal constitution of the outer crust o...
The properties of the crust of a neutron star can be significantly altered by the presence of a high...
Magnetars form a subclass of neutron stars characterized by magnetic fields of order 1014-1015 G at ...
Magnetic fields of order 10^15 G have been measured at the surface of some neutron stars, and much s...
A very fast iterative method is presented to calculate the internal constitution of the outer crust ...
This computer code (written in C language) determines the internal constitution of the outer crust o...
The outer-crust structure and composition of a cold, non-accreting magnetar are studied. We model th...
With observed surface magnetic fields up to ∼10^15 G, neutron stars - the stellar remnants of gravit...
Magnetars are neutron stars endowed with surface magnetic fields of the order of $10^{14}-10^{15}$~G...
The role of a strong magnetic field on the neutron-drip transition in the crust of a magnetar is stu...
International audienceIn this work, we compute the structure and composition of the inner crust of a...
Current models of magnetars require extremely strong magnetic fields to explain their observed quies...
International audienceIn this review we discuss self-consistent methods to calculate the global stru...
We have studied various physical properties of magnetically deformed atoms and the associated matter...
Isolated neutron stars show a diversity in timing and spectral properties, which has historically le...
This computer code (written in C language) determines the internal constitution of the outer crust o...
The properties of the crust of a neutron star can be significantly altered by the presence of a high...
Magnetars form a subclass of neutron stars characterized by magnetic fields of order 1014-1015 G at ...
Magnetic fields of order 10^15 G have been measured at the surface of some neutron stars, and much s...
A very fast iterative method is presented to calculate the internal constitution of the outer crust ...
This computer code (written in C language) determines the internal constitution of the outer crust o...
The outer-crust structure and composition of a cold, non-accreting magnetar are studied. We model th...
With observed surface magnetic fields up to ∼10^15 G, neutron stars - the stellar remnants of gravit...
Magnetars are neutron stars endowed with surface magnetic fields of the order of $10^{14}-10^{15}$~G...
The role of a strong magnetic field on the neutron-drip transition in the crust of a magnetar is stu...
International audienceIn this work, we compute the structure and composition of the inner crust of a...
Current models of magnetars require extremely strong magnetic fields to explain their observed quies...
International audienceIn this review we discuss self-consistent methods to calculate the global stru...
We have studied various physical properties of magnetically deformed atoms and the associated matter...
Isolated neutron stars show a diversity in timing and spectral properties, which has historically le...